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CY 11001 CHEMISTRY

Professor: Dr. Amita (Pathak) Mahanty
Office:    Room C-301 (2nd Floor, Chemistry Department)
e-mail:    ami@chem.iitkgp.ernet.in
phone:     83312 (office)

Ground Rules for the Class
• Mobile Phones in switched off mode
• Attendance is a must and will be checked regularly
• Vast syllabus and fast paced, advised to take class notes
SCHEDULE CHEMISTRY THEORY COURSE
              SECTIONS 1, 2 & 3
Physical: 3rd Jan, 2013 – 1st Feb, 2013 (11 lectures)

Inorganic: 7th February, 2013- 15th March, 2013 (12 lectures)
MID TERM SEMESTER EXAM … 18.02.2013 - 26.02.2013
                         (Monday -Tuesday)
Organic: 18th March, 2013 - 12th April, 2013 (12 classes)


                    Room No.       Day      Time
                               Monday       4:30-5:25
                      F-116    Thursday     4:30-5:25
Lecture Timings:
                               Friday       4:30-5:25
Tutorial Schedule for Spring 2012-13
Sec &      Tutorial    Tutorial    Tutorial              Roll No
Group      Room         Day        Timings
           No                       (AM)
Sec: 11A    S-126     Thursday    10:30-11.25 AE, AG, BT, CE, CH, CS,
                                              CY
Sec: 11B    S-127     Thursday    10:30-11.25 EC, EE, EX, GG, HS, IE,
                                              IM, MA, ME10008
Sec: 11C    F-131     Thursday    10:30-11.25 ME10022, MF, MI, MT, NA,
                                              PH, QD


Sec: 12A    S-126     Monday      8.30 - 9.25   AE, AG, BT, CE, CH, CS,
                                                CY20010
Sec: 12B    S-127     Monday      8.30 - 9.25   CY20024, EC, EE, EX, GG,
                                                HS, IE, IM, MA20032
Sec: 12C    F-131     Monday      8.30 - 9.25   MA20046, ME, MF, MI, MT,
                                                NA, PH, QD
CY 11001 CHEMISTRY

Distribution of Marks:
Mid Semester Exam (Only Physical): 30%
End Semester Exam (Inorganic & Organic): 50%

Teachers Assessment (TA): 20%
Break up: [Physical (6%), Inorganic (7%), Organic (7%)]

TA marks to be based on a CLASS-TEST: 30th January 2013

Text Book:
Atkin’s Physical Chemistry 8th Ed

Reference Books:
Physical Chemistry by Silbey, Alberty & Bawendy; Wiley.
Physical Chemistry by I. N. Levine; McGrew.
Physical Chemistry David W. Ball; Thompson.
CY 11001 CHEMISTRY (L-T-P : 3-1-0; Credit : 4)
Thermodynamics of Chemical Processes:
    • Review of Essential Concepts and Definitions
      • Revision: Heat, Work & Energy; First Law of Thermodynamics
      • The Second Law of Thermodynamics • Concept of Entropy
      • Gibbs Free Energy       • Equilibrium conditions for Closed Systems
      • Maxwell Relations       • The Chemical Potential
      • Definition and Concept of Open Systems
      • Phase and Reaction Equilibria

Electrochemical Systems:
     • Electrochemical Cells and EMF
     • Applications of EMF Measurements: Thermodynamic data,
       Activity Coefficients, Solubility product and pH

Kinetics of Chemical Reactions:
     • Reversible, Consecutive and Parallel Reactions,
      • Steady State Approximation,
      • Chain Reactions, Photochemical Kinetics
Thermodynamic

Thermodynamics provides a framework of relating the macroscopic
properties of a system to one another.
Thermodynamic: ↔ Classical, Statistical and Irreversible
Classical Thermodynamics, to the study of macroscopic properties of
system/matter at equilibrium using the laws governing transformation
of energy from one form to another.
It is concerned only with macroscopic quantities and ignores the
microscopic variables that characterize individual molecules.

THE BASIC CONCEPTS:
  System, the part of the world in which we have a special interest.
  Surroundings, the region outside the system where we make our
measurements.
  Boundary, a hypothetical/real barrier between system and
surroundings.
Thermodynamic Systems

Open systems can exchange both matter
and energy with the environment.
Closed systems exchange energy but not
matter with the environment.
Isolated systems can exchange neither
energy nor matter with the environment.
Thermodynamic Systems


   System : Open, Closed, Isolated
   Surroundings
   Boundary / Wall
   • Rigid and Non rigid (movable)
   • Permeable and Impermeable (no matter is allowed to pass
     through it)
   • Adiabatic and Diathermic boundary ( - permits the passage of
     energy as heat )


A system surrounded by a rigid, impermeable, adiabatic wall –
Isolated system Example: Universe as a whole, a thermo flask
Thermodynamic Equilibrium

 For Isolated system:
• Macroscopic properties do not change with time

 For Non isolated system:
a) Macroscopic properties do not change with time
b) Removal of the system from contact with its surroundings causes
 no change in the properties of the system


• A system in thermodynamic equilibrium is an equilibrium system
• Thermodynamic State only defined by the present values of the
  state variables, not by the history

      What are conditions of Thermodynamic Equilibrium?
Mechanical equilibrium


The condition of equality of pressure on
either side of a movable wall / boundary.

No unbalanced forces act on or within
the system – does not undergo
acceleration or no turbulence inside the
system
Thermal equilibrium


Thermal equilibrium between system and
the surroundings, is a condition in which
there is no change in the properties of the
system or surroundings when they are
separated by a thermally conducting wall.

In other words, Thermal Equilibrium is a
condition in which no change of state occurs
when two objects A to B are in contact
through a diathermic boundary.
Material Equilibrium

Concentrations of the chemical species in the various parts of the
system are constant with time
a) No net chemical reactions are occurring in the system
b) There is no net transfer of matter from one part (phase) of the
   system to another or between the system and its surroundings
   Phase: a homogeneous part of a system is called a phase

 For thermodynamic equilibrium, all three kinds of equilibrium
 must be present
 No matter what is the initial state of an isolated system,
 eventually it will reach the state of thermodynamic equilibrium
How do we define a system? State of a System

Macroscopic state of a system can be specified by the values of a small
number of macroscopic Properties/Parameters/Physical characteristics or
attributes of a system - Thermodynamic variables

Thermodynamic variables which are experimentally measurable
• Composition – mass of each chemical species that is present in each
  phases,
• pressure (P), volume (V), Temperature (T), density, etc.
• field strength, if magnetic/electrical field act on the system
• gravitational field
(N.B.: only the average values are considered, all fluctuation and
  perturbations are ignored).

On the other hand, Microscopic state of a system needs description of each
molecule – a very complicated picture
Thermodynamic State

If the value of every thermodynamic property in system A is same as in
system B – then they are in the same thermodynamic state

The state of a thermodynamic system is defined by specifying the values of
its thermodynamic properties – However, it is not necessary to specify all
the properties to define the state of a system.

In fact, the macroscopic state of a system can be specified by the values of
a small number of macroscopic variables – these called the Properties /
Parameters / Thermodynamic variables of a system.

For instance: The thermodynamic state of a single-phase system of fixed
amounts of non reacting substances can be described by any two of the
three state functions (P, V and T)

Equation of state, an equation that interrelates pressure, volume,
temperature, and amount of substance: P = f (T, V, n).
The Equation of State of Ideal Gases
An equation of state - an equation that relates macroscopic variables (e.g.,
P, V, and T) for a given substance in thermodynamic equilibrium.
In equilibrium (≡ No macroscopic motion), just a few macroscopic
parameters are required to describe the state of a system.

Geometrical representation of the equation of state: f (P,V,T) = 0
The ideal gas equation of state: PV = nRT
                                                               an equilibrium
                                                          P         state

P   –   pressure                           [Newtons/m2]
V   –   volume                             [m3]
                                                                        the equation-
n   –   number of moles of gas                                         of-state surface
T   –   the temperature in Kelvins         [K]
                                             J
R – a universal constant        R ≈ 8.31                              V
                                           mol ⋅ K
                                                          T
Recap
The gas laws
     Boyle’s law: At constant temperature, the pressure of a
     sample of gas is inversely proportional to its volume, p ∝
     1/V at constant temperature.
     Charles’ law: At constant pressure, the volume of a gas is
     proportional to the absolute tem perature, V ∝ T at constant
     pressure.
     Avogadro’s principle: Equal volumes of gases at the same
     pressure and temperature contain the same numbers of
     molecules.

     Dalton’s law: The pressure exerted by a mixture of gases is
     the sum of the partial pressures of the gases.
Thermodynamic Systems
   Homogeneous system, a system having its properties uniform
throughout – a single phase solution / pure.

  Heterogeneous system, a system with more than one phase.

Intensive properties
  Does not depend upon size (the quantity/amount of matter present) of
  the system [e.g. Pressure, Temp, Viscosity, Density etc.]
  Total Property = property of part of the system
Extensive properties
  Depends upon size of the system [e.g. n, V, surface area etc ]
  Extensive properties depend on the amount of substance in the system.]
  Total Property = Σ property (in each part of the system)

Other variables:
Compositions, Surface area, Electrical/magnetic strength
Gravitational field can/are generally ignored
A very important macroscopic parameter: Temperature

 Temperature is a property associated with random motion of
 many particles. Introduction of the concept of temperature in
 thermodynamics is based on the the 0’th law of thermodynamics:




  B acts as Thermometer.
  A, B, C all are at the same “temperature”.

A well-defined quantity called Temperature exists such that two
systems will be in thermal equilibrium if and only if both have the
same temperature.
Thermodynamic State Variables / Properties
Thermodynamic State Variables / Properties




    Therefore, For describing the State of a System we require:
• A few experimentally measureable macroscopic properties: p, T, V, n, m, ...
• Knowledge if System is Homogeneous or Heterogeneous
• Knowledge if System is in Equilibrium State
• Knowledge of the number of components
Thermodynamic Process: Operation for Change in State
Change of State: Transformation
e.g.,   3 H2 (g, 5 bar, 100 °C) → 3 H2 (g, 1 bar, 50 °C)
        (initial state)           (final state)
Path:   Sequence of Intermediate states through which a system passes
        to attain the final state

Process: Operation through which a system undergoes a change in state.
         Process describes the path.
                                                           Path
Path can be:
  Reversible (always in Equilibrium)
  Irreversible (describes direction of time)
  Cyclic(initial and final state have the same value)
Processes can be:
• Adiabatic (No heat transfer between system and surrounding)
• Isobaric (Constant pressure process)
• Isothermal (Constant temp process)
• Constant Volume process • Endothermic & Exothermic process (q<0 & q>0)
Essential concepts / Definitions
Processes : When one or more of the parameters of a system changes, the
state of the system also changes and the system is said to have undergone
a process.
 Various types of processes:
 • Isothermal (T),
 • Isobaric (P),
 • Isochoric (V)
 • Adiabatic (q),
 • Isenthalpic (H)
 • Exothermic & Endothermic
 • Cyclic


  Each process can be
  either carried out
  Reversibly or
  Irreversibly
Thermodynamic Processes can be :
Reversible process: Ideal process
• Change must occur in successive stages of infinitesimal quantities
• Infinite duration
• Virtual thermodynamic equilibrium, at each of the small stages.
• Changes of the thermodynamic quantities in the different stages will be
  the same as in the forward direction but opposite in sign w.r.t. forward
  direction. The system and surroundings can be put back in their original
  states by exactly reversing the process.
Irreversible Process: Real / Spontaneous
• Occurs suddenly or spontaneously without the restriction of occurring in
  successive stages of infinitetesimal quantities. Irreversible processes
  cannot be undone by exactly reversing the change to the system.
• Do not remain in the virtual equilibrium during the transition.
• The work (w) in the forward and backward processes would be unequal.
Cyclic process: • Is one in which the initial and final states are the same.
  In such process:
• There is no change in the state variables (e.g., ∫dU = Uf-Ui = 0)
• In contrast, path functions generally have non-zero values for cyclic
  processes, dependent on the path (e.g., ∫δw ≠ (wf – wi) ≠ 0]
Spontaneous Processes



•   Spontaneous processes are those
    that can proceed without any
    outside intervention.

•   The gas in vessel B will
    spontaneously effuse into vessel
    A, but once the gas is in both
    vessels, it will not spontaneously
    go back to B
Reversible Processes

           In a reversible process the
           system changes in such a way
           that the system and
           surroundings can be put back
           in their original states by
           exactly reversing the process.

           Changes are infinitesimally
           small in a reversible process.
Irreversible Processes




• Irreversible processes cannot be undone by exactly reversing
  the change to the system.
• All Spontaneous processes are irreversible.
• All Real processes are irreversible.
Energy, Work and Heat
    Energy is the capacity to do work.

    Energy classification into:    kinetic       potential
                                   (by motion)   (by position)
    Is purely arbitrary!           e.g.thermal   chemical, electrical

•   Heat and work are NOT “types” of ENERGY, but are processes involving
    TRANSFER of energy.

•   They appear and disappear at the system boundary. They are path variables.
•   Heat is the transfer of energy from one body to another based on temperature
    difference. They are path variables.
•   Heat stimulates random motion.
•   Convention: if heat flows into the system, q > 0.

•   Work is the transfer of energy by some mechanism other than temperature
    difference.
•   They appear and disappear at the system boundary. They are path variables.
•   Convention: if work is done on the system, w > 0.
•   Work stimulates organized motion.
•   Work “degrades” into heat.

    Qualitative observations by Count Rumford (Ben Thompson)
    Quantitative measurements by James Joule
Energy
  Concept of Internal Energy

• E = K + V + U    where, K and V are the macroscopic (not
  molecular) kinetic and potential energies of the system

• U is the internal energy of the body (due to molecular motions
  and intermolecular interactions)

• Internal Energy,U, is the total kinetic energy due to motion of
  molecules (translational, rotational, vibrational) the total potential
  energy associated with the vibrational and electric energy of
  atoms within molecules or crystals.

• Um (molar internal energy) = U/n, where n= no. of moles of the
  substance

• Um = Utr, m + Urot, m + Uvib, m + Uinternal, m + Urest, m (where,
  Urest,m = rest mass energy of electrons & nuclei = mrelC2= constant)
Energy

 Properties of Internal Energy

• U is a State function, a property that: Depends only on the
  current state of the system and is independent of how or
  through path that state has been reached.

• It is an exact differential and its fundamental variables are
  V and T              ⎛ ∂U ⎞     ⎛ ∂U ⎞
  U = f (V, T);   dU = ⎜
                         ∂V
                            ⎟ dV +⎜
                                    ∂T
                                       ⎟ dT
                        ⎝      ⎠T       ⎝   ⎠V


• For cyclic process,       ∫ dU   =0

• U is an Extensive property
The First Law of Thermodynamics: Work, Heat & Energy




  T1 → T2




  T1 → T2              h




 Joule Experiment
                     Joule Equivalent of Heat:   1 cal = 4.184 J
Work
• Expansion work, work of expansion (or compression)
• Non-expansion / additional work: any other work

                        where




 •   pex = external pressure
 •   A = piston area
 •   dz = displacement
 •   dV = Adz = volume change for the gas
                             vf

 Total work done,     w = − ∫ p ex dV
                             vi

• Work done on the system         + ve i.e., Compression

• Work done by the system         - ve   i.e., Expansion
1st Law of Thermodynamics
Consider an example system of a piston and
cylinder with an enclosed dilute gas
characterized by P,V,T & n.

What happens to the gas if the piston is moved
inwards? Compression

•If the container is insulated the temperature
will rise, the atoms move faster and the
pressure rises.

•Is there more internal energy in the gas? Yes
                                                 ∆x
External agent did work in pushing the piston
inward.
w = - F     d    = -(PA)    (-Δx)
w = P Δ V

Work done on the gas equals the change in the
internal energy of the gas w = Δ U
1st Law of Thermodynamics

• Change the situation:
• Keep the piston fixed at its
  original location.
• Place the cylinder on a hot plate.

What happens to gas?
• Heat flows into the gas.
• Atoms move faster, internal energy
  increases.
• Q = heat (in Joules) flows in
  ∆U = change in internal energy in
  Joules.
  Q = ∆U
1st Law of Thermodynamics
                                                    F
 What if we added heat and pushed the piston
 in at the same time?

 • Work is done on the gas,
 • Heat is added to the gas and
 • the internal energy of the gas
   increases:
    ΔU = w + Q


U INCREASES with INCREASE in TEMP. of the system, when:
1. work is done on the system by the surrounding or,
2. heat flows into the system from the surrounding or,
3. both, heat and work flows from the surr. into the system
The First Law: Sign convention

• Work done on the system by surr   + ve   i.e., Compression

• Work done by the system by surr   - ve i.e., Expansion
Partial Differentiation: A primer

Consider a function of two variables    f (x,y)

Definition: A partial derivative of one of the
variables: the rate of change of the function
w.r.t. that variable with all other variables
kept fixed.

Suppose: f = f (x,y),

⎛ df ⎞            f ( x + Δx,y ) − f ( x,y )
⎜ dx ⎟ = LimΔx →0
⎝    ⎠y                      Δx
⎛ df ⎞             f ( x ,y + Δy ) − f ( x,y )
⎜    ⎟  = LimΔy →0
⎝ dy ⎠x                        Δy

• For example: f (x, y) = x2y          ⎛ ∂f ⎞        ⎛ ∂f ⎞
                                       ⎜∂ ⎟   = 2xy, ⎜ ⎟ = x 2
                                       ⎝ x ⎠y        ⎝ ∂y ⎠x
Properties of partial derivatives

Consider a function of two variables      f (x, y)
∴ Its differential form will be:

     ⎛ df ⎞      ⎛ df ⎞
df = ⎜    ⎟ dx + ⎜ dy ⎟ dy
     ⎝ dx ⎠ y    ⎝    ⎠x

•The   Chain rule:

Let s be an independent parameter and if change of s results in
changes in the values of x and y.

i.e., x = x (s); y = y (s);   ∴ we can write, f (x, y) ≡ f (s)

 df   ⎛ df ⎞ dx     ⎛ df ⎞ dy
    = ⎜    ⎟      + ⎜    ⎟
 ds   ⎝ dx ⎠ y ds   ⎝ dy ⎠ x ds
Properties of partial derivatives
• The Cyclic Rule:

If z is a function two variable, then we can write: z = z (x, y),
       ⎛ dy ⎞ ⎛ dz ⎞       ⎛ dx ⎞
 then, ⎜                   ⎜    ⎟ = −1
       ⎝ dz ⎟ x ⎜ dx ⎟ y
            ⎠ ⎝      ⎠     ⎝ dy ⎠ z

 Example:
 If V = f (p, T);    p = f (V, T);       T= f (p, V), then we can write
⎛ dp ⎞ ⎛ dT ⎞ ⎛ dV ⎞
⎜    ⎟ ⎜     ⎟ ⎜      ⎟ = −1
⎝ dT ⎠V ⎝ dV ⎠ p ⎝ dp ⎠T

Example 1:                                ⎛ dp ⎞    nR ⎛ dT ⎞    p ⎛ dV ⎞    nRT
                                          ⎜ dT ⎟  =   ;⎜    ⎟  =  ;⎜    ⎟  =− 2
                                          ⎝    ⎠V   V  ⎝ dV ⎠ p nR ⎝ dp ⎠T    p
Use the Equation of state for
Ideal gas to verify the cyclic             ⎛ dp ⎞ ⎛ dT ⎞ ⎛ dV ⎞     ⎛ nR ⎞ ⎛ p ⎞ ⎛ nRT ⎞
                                          ∴⎜    ⎟ ⎜     ⎟   ⎜    ⎟ =⎜    ⎟⎜    ⎟ ⎜− 2 ⎟
rule                                       ⎝ dT ⎠V ⎝ dV ⎠ p ⎝ dp ⎠T ⎝ V ⎠ ⎝ nR ⎠ ⎝ p ⎠
p = nRT/V; V= nRT/p; T= pV/nR                ⎛ nRT ⎞
                                          = −⎜     ⎟ = −1
                                             ⎝  pV ⎠
Properties of partial derivatives

•Two partial derivatives operating on a function:
 Let f be function of two variables, i.e., f = f (x, y);
 Double partial derivative of the function f can be written as:
   ∂ ⎛ df ⎞    ∂ 2f         ∂2f      ∂2f
     ⎜    ⎟ =                     =
  ∂x ⎝ dy ⎠ x ∂ x ∂y       ∂x ∂ y   ∂ y ∂x


 Verification: Let the function be: f ( x , y ) = x 2 y ,
                 ∴
   ∂ f
    2
                  ∂ 2f                The exact differential
        = 2x,          = 2x,
  ∂y ∂x          ∂y ∂x



•In general, the total differential form of f(x,y) may be written as:
  df = M( x , y )dx + N ( x , y )dy
   where , M = ⎛ ∂f ⎞             and            ⎛ ∂f ⎞
                                             N = ⎜
               ⎜    ⎟                                 ⎟
                       ⎝ ∂x ⎠ y                  ⎝ ∂y ⎠ x
Properties of partial derivatives

• Does any differential form of type [M(x,y)dx + N(x,y)dy]
  always represent the total differential form of a function?

  Only if           ⎛ ∂M ⎞     ⎛ ∂N ⎞
                    ⎜    ⎟   = ⎜    ⎟
                    ⎝ ∂y ⎠ x   ⎝ ∂x ⎠ y
Then, df = [M(x,y)dx + N(x,y)dy] represents an exact differential.


Example:
Let us consider: 3 x 2 y 2 dx + 2 x 3 ydy   where,
 M( x , y ) = 3 x 2 y 2 ,
 N ( x ,y ) = 2 x 3y
 It can be easily verified that the above expression corresponds
 to an exact differential function of the type:

 3 x 2 y 2 dx + 2 x 3 ydy = d ( x 3 y 2 )
Properties of partial derivatives

 Consequence:
 Let us move from a point (xi,yi) to another point (xf,yf)
 The corresponding change in f(x,y) can be written as:
                                        f          f
 Δf = f ( xf , yf ) − f ( xi , yi ) =   ∫ df
                                        i
                                               =   ∫ ( Mdx
                                                   i
                                                             + Ndy )


• The VALUE OF THE INTEGRAL OF AN EXACT DIFFERENTIAL is
  INDEPENDENT OF THE PATH taken in going from initial to final
  point and DEPENDS only on the values of f(x, y) at the initial and
  the final points.


NOTE:
Integral of an exact differential function,df, for a closed path
(i.e., cyclic) where, i (initial state) = f (final state): ∫ df = 0
Test for Exactness (State Variable)

If z = f( x,y),                             dz will be a perfect differential
                                             when it is found
               ∂z ⎞        ⎛∂z ⎞
then , dz = ⎛
            ⎜      ⎟  dx + ⎜ ⎟ dy
             ⎝ ∂ x ⎠y      ⎝ ∂ y ⎠x         • dz is a single-valued function
      ∂z             ⎛ ∂z ⎞                  depending entirely on the
if, ⎛ ⎞ = M ; and ⎜ ⎟ = N
    ⎜ ⎟                                      instantaneous values of x and y.
    ⎝ ∂x ⎠y          ⎝ ∂y ⎠x
then, dz = M( x,y)dx + N( x,y)dy            • dz between any two specified
                                             points or states is independent of
                                             the path of transition.
Then for exact differential,
 ⎛ ∂ M⎞     ⎛ ∂N ⎞                          • dz for a complete cyclic process
⇒⎜     ⎟  = ⎜     ⎟                          is equal to zero
 ⎝ ∂ y ⎠x   ⎝ ∂ x ⎠y
      ⎡ ∂ ⎛∂z ⎞ ⎤        ⎡ ∂ ⎛∂z ⎞ ⎤        • δq and δw are NOT EXACT
i.e., ⎢ ⎜ ⎟ ⎥ =          ⎢ ⎜ ⎟ ⎥             differential quantities therefore
      ⎣∂ y ⎝ ∂ x ⎠y ⎦x   ⎢∂ x ⎝ ∂ y ⎠x ⎦y
                         ⎣             ⎥     they are NOT STATE Variables.
Properties of partial derivatives
The gas laws
    isotherm, curves in a graph corresponding to a single
    temperature.
    isobar, curves in a graph corresponding to a single pressure.
    isochore, curves in a graph corresponding to a single
    volume.
    gas constant, R (with R = NAk, where NA is Avogadro’s
    constant and k is Boltzmann’s constant).
The gas law

        perfect/ideal gas equation, pV = nRT.
        perfect/ideal gas, a gas that obeys pV = nRT exactly under
        all conditions.
        real gas, an actual gas. e.g.,
        standard ambient temperature and pressure (SATP),
        298.15 K (25 °C) and 1 bar (or, 0.986 atm or 100 kPa).
        standard temperature and pressure (STP)
        273.15 K (0 °C) and 1 bar (100 kPa, 0.986 atm.)
        Normal temperature and pressure (NTP)
        273.15 K (0 °C) and 1 atm (101.325 kPa, 760 Torr)

1 atm =(101.325 kN/m2, 101.325 kPa, 14.7 psi, 29.92 in Hg, 760 torr).
Partial pressure , of a gas is the pressure the gas would exert if it
occupied the container alone; in general, pi = xi P


Vapour pressure, the pressure of a vapour in equilibrium with its
condensed phase

Mole fraction, the amount of i species, expressed as a fraction of moles
of the moles of ith species (ni) to the total amount of moles, n, in the
sample, xi = ni/n
partial pressure: of an ideal gas, the pressure a gas would
exert if it occupied the container alone; in general, pi = xi p.
Dalton’s law: The pressure exerted by a mixture of gases is
the sum of the partial pressures of the gases.
Thermodynamics

          Thermodynamics:
          → Describes macroscopic    properties of equilibrium
              systems
          →   Entirely Empirical

          →   Built on 4 Laws and “simple” mathematics



           0th Law      Defines Temperature (T)
           1st Law      Defines Energy (U)
           2nd Law      Defines Entropy (S)
           3rd Law      Gives Numerical Value to Entropy




These laws are UNIVERSALLY VALID, they cannot be circumvented
Work
• Expansion work, work of expansion (or compression)
• Non-expansion / additional work: any other work

                        where




 •   pex = external pressure
 •   A = piston area
 •   dz = displacement
 •   dV = Adz = volume change for the gas
                            vf

 Total work done,     w = − ∫ p ex dV
                            vi

• Work done on the system        + ve i.e., Compression

• Work done by the system        - ve   i.e., Expansion
1st Law of Thermodynamics
                                                                       F
 Consider an example system of a piston and
 cylinder   with   an   enclosed dilute gas
 characterized by P,V,T & n.
 What if we added heat and pushed the piston
 in at the same time?
 • Work is done on the gas,
 • Heat is added to the gas and
 • the internal energy of the gas
   increases:
   ΔU = w + Q
Statement: Change of internal energy in a closed system of is equal to the energy
flow across its boundary as heat or work

 U INCREASES with INCREASE in TEMP. of the system, when:
 1. work is done on the system by the surrounding or,
 2. heat flows into the system from the surrounding or,
 3. both, heat and work flows from the surr. into the system
The First Law: Sign convention
  • Work done on the system by surr      + ve   i.e., Compression

  • Work done by the system by surr      - ve i.e., Expansion




Alternate Statement: If a system is subjected to a CYCLIC
Transformation, the work produced in the surroundings is equal to
the heat withdrawn from the surroundings.

        Q = -w (change in U is zero as it’s a State function)
If w is +ve (compression, work done on the system) then q will be –ve
(heat will be released by the system) and vice versa
Work
• Expansive work, work of expansion (or compression)
• Non-expansive / additional work : any other work

                 piston held down by
F= mg                           pins
pex= mg/A
F= pex.A


          m       dz

Area =A

Pi , Vi             Pf , Vf

w = - mg.A.dz
w = - mg.dV
w = - pex.dV =-pex (Vf-Vi)
WORK
Reversible Isothermal Expansion :
            w = − ∫ ( pex − dp)dV = − ∫ ( pdV − dpdV ) = − ∫ pdV
                       dV           Vf               where, p = p(V)
            w = −nRT ∫    = −nRT ln                  p = nRT/V
                       V            Vi

                              Irreversible Isothermal Expansion:
                                       Vf

                              w = − pex ∫ dV = − pex (V f − Vi ) = − pex ΔV
                                        Vi
Irreversible




 Irreversible
Irreversible                                 Reversible

Expansion




              Irreversible


                                                            Reversible


Compression



     • For a reversible process Work on expansion = work of compression
     (same path)
     • For an irreversible process Work on expansion ≠ work of compression
     (same path)
Work




 wrev    >   wirr

• Work done on expansion by the system on surroundings (sign negative)
operating between specified initial and final states and passing through
and specified path is maximum work available from a system when the
changes take place reversibly
• For a reversible process Work on expansion = work of compression
(same path)
• For an irreversible process Work on expansion ≠ work of compression
(same path)
• Work is a path dependent parameter, path function(so as Heat)
State and Path Functions

•   Some state functions, e.g., U and H etc.
     – Value of a state function is independent of                         Path 2 - Non-
       path                                                                  adiabatic
                                                                             w≠0;q≠0
     – Depends only on initial and final state,             Path 1 -
       e.g. ΔU = Ufinal - Uinitial                         Adiabatic
                                                           w≠0;q=0
     – Overall Change
             final
    ΔU = ∫           dU ⇒   dU is an exact differential
          initial




•   Path from initial to final state has a functional
    dependence
     – For ∆U, work may be done, or, heat may
       flow or, both
     – Equations that describe how you get to final       ΔUpath1 = ΔUpath2 = Uf -Ui
       state are path functions
     – Path functions are path specific

                        ∂q ⇒ ∂q is
          final
    q=∫                              an inexact differential
         initial,path
Work is a STATE FUNCTION?

  Assume a Reversible process so that pext = p where, Ar (gas)
  under goes change of state through compression, from
  Ar (g, p1, V1) (initial) → Ar (g, P2, V2) (final);
  such that V1 > V2 and p1< p2




Compression through two paths

1st Path:
Ar(g, p1, V1) → Ar(g, p1, V2) → Ar(g, p2, V2)
First V1 → V2 when p held constant at p1;
then p1 → p2 when V held constant at V2

2nd Path:
Ar(g, p1, V1) → Ar(g, p2, V1) → Ar(g, p2, V2)
First p1 → p2 when V held constant at V1;
then V1 → V2 when p held constant at p2

Note for the closed cycle, total work = w[path (1)] - [path (2)]
Work is a STATE FUNCTION?
                                      V2         V2

                          w( 1) = − ∫ pextdV − ∫ pextdV
                                      V1         V2

                                      V2

                          w( 1) = − ∫ p1dV = − p1(V − V ) = p1(V − V )
                                                   2   1        1   2
                                      V1

                                      V1         V2

                          w( 2 ) = − ∫ pextdV − ∫ pextdV
                                      V1         V1

                                      V2

                          w( 2 ) = − ∫ p2dV = − p2 (V − V ) = p2 (V − V )
                                                     2   1         1   2
                                      V1

NOTE:
• Work done on the system to compress it is NOT EQUAL through
  the two paths. i.e., w(1) ≠ w (2)
• ∴ Net work done on the system in the complete cycle ≠ 0
   i.e., [w(1) - w(2)] ≠ 0;   ∫ ∂w ≠ 0 (closed cycle)
• This means w is NOT a state function ∴ we CAN NOT write
  w = f(V, p)
Ideal gas, closed system, reversible process
Calculate         wf and wb

                      isothermal
10 Pa, 1   m3 ,   T                1 Pa, 10 m3, T




              isochoric
10 Pa, 1 m3, T          1 Pa, 1 m3, T2

                                     1 Pa, 10 m3, T
                          isobaric

                  isobaric
10 Pa, 1 m3, T                10 Pa, 10 m3, T3


                                         1 Pa, 10 m3, T
                             isochoric
25 L of gas is enclosed in a cylinder/piston apparatus at
2 atm of pressure and 300 K. A 100 kg of mass is
placed on the piston causing the gas to compress to 20 L
at constant pressure. This is done by allowing heat to
flow out of the gas. What is the work done on the gas?
What is the change in internal energy of the gas? How
much heat flowed out of the gas?
•   Po = 202,600 Pa,   Vo = 0.025 m3,
•   To = 300 K,        Pf = 202,600 Pa,
•   Vf=0.020 m3,       Tf= ?

•   n = PV/RT    W = -P∆V      ∆ U = 3/2 nR ∆T   Q = W + ∆ U

W = - P ∆ V = -202,600 Pa (0.020 – 0.025)m3
  = 1013 J energy added to the gas

∆ U =3/2 nR ∆T=1.5(2.03)(8.31)(-60)= -1518 J

Q = W + ∆ U = 1013 – 1518 = -505 J heat out
Heat Transactions

 In general change in the internal       dU = dq + dw exp + dw add
 energy of a closed system is given by

- For dV = 0; dwexp = 0 and if dwadd = 0, then
 dU = dq (constant volume, no additional work) = dqv

 For a measurable change, ΔU = qv
-heat capacity, C, the ratio of heat supplied to
 the temperature rise it causes. C = dq/dT;
                                 C = q/ ΔT

- heat capacity at constant volume, CV = (∂U/∂T)V

- molar heat capacity, the heat capacity divided
by the amount of substance, Cm = C /n.                 adiabatic bomb
                                                       calorimeter
- specific heat capacity, the heat capacity
divided by the mass, Cs = C /m
Heat Capacity for Constant Volume Processes (Cv)



       insulation                           ΔT

                                 Heat, Q
                      m          added           m


• Heat is added to a substance of mass m in a fixed volume
  enclosure, which causes a change in internal energy, U. Thus,

                    Q = U2 - U1 = ∆U = m Cv ∆T

  The v subscript implies constant volume
Heat Capacity for Constant Pressure Processes (Cp)


                            Δx
                               ΔT

                       Heat, Q
          m            added                  m



• Heat is added to a substance of mass m held at a fixed
  pressure, which causes a change in internal energy, U,
  AND some PV work.
Heat Transactions and Enthalpy

For dV ≠ 0; dwexp≠ 0 even if dwadd = 0, then          dU ≠ dq
ΔU = qp - pΔV  qp = ΔU +pΔV = U2 – U1 + p(V2 – V1)
                               = (U2 + pV2) – (U1 + pV1)
Define H = U + pV
                                       •Differential scanning calorimeter
dH = dU + pdV + Vdp                    •Isobaric calorimeter
   = dU - w (at constant p)            •Adiabatic flame calorimeter
   = dqp
 At constant p, dH = dqp (constant pressure, no additional work)

- Heat capacity at constant pressure, Cp = (∂H/∂T)p

- Enthalpy change and temperature change, dH = nCp,m dT;
                                       ΔH = nCp,m ΔT (if Cp independent of T)


Empirical expression,
Cp,m = a + bT + c/T2
Heat Transactions
- for ideal/perfect gas; relation between ∆U and ∆H,
            ∆H = ∆U + ∆ngRT.

- relation between heat capacities of a perfect gas,
            Cp – CV = nR
For any process

U = f (V , T )                     H = f ( P, T )
     ⎛ ∂U ⎞
dU = ⎜
                 ⎛ ∂U ⎞
          ⎟ dV + ⎜
                                        ⎛ ∂H ⎞         ⎛ ∂H ⎞
                      ⎟ dT         dH = ⎜     ⎟ dP + ⎜      ⎟ dT
     ⎝ ∂V ⎠T     ⎝ ∂T ⎠V                ⎝ ∂P ⎠ T       ⎝ ∂T ⎠ P
    = π T dV + CV dT                   ⎛ ∂H ⎞
                                      =⎜    ⎟ dP + C P dT
        ⎛ ∂U ⎞                         ⎝ ∂P ⎠T
   πT = ⎜    ⎟ Internal pressure
        ⎝ ∂V ⎠ T

dU = CV dT (for ideal gas)         dH = Cp dT (for ideal gas)
For ideal gas         ⎛ ∂U ⎞       For ideal gas
                 πT = ⎜    ⎟ =0                     ⎛ ∂H ⎞
                      ⎝ ∂V ⎠T                       ⎜    ⎟ =0
                                                    ⎝ ∂P ⎠T
            Joule Experiment
Adiabatic Reversible Process for ideal gas,
                  Cv independent of Temp
                                                                            1
dU = dw + dq = dw
                                   CV                 nR
                          ⎛ T2 ⎞         ⎛ V1 ⎞            T2 ⎛ V1 ⎞        C
                          ⎜ ⎟           =⎜ ⎟
                                                                            c

                          ⎜T ⎟           ⎜V ⎟                = ⎜ ⎟ where c = V ,m
Cv dT = − pdV             ⎝ 1⎠           ⎝ 2⎠              T1 ⎜ V2 ⎟
                                                               ⎝ ⎠           R
                                   CV            nR            C p −CV
    T2 dT         V2 dV   ⎛ T2 ⎞         ⎛V ⎞          ⎛V ⎞
Cv ∫      = - nR ∫        ⎜ ⎟
                          ⎜T ⎟          =⎜ 1 ⎟
                                         ⎜V ⎟         =⎜ 1 ⎟
                                                       ⎜V ⎟
    T1 T          V1 V    ⎝ 1⎠           ⎝ 2⎠          ⎝ 2⎠
                                          γ −1
     T2       V1          T2 ⎛ V1 ⎞                                C p ,m
Cv ln = nR ln               =⎜ ⎟                 where γ =
     T1       V2          T1 ⎜ V2 ⎟
                             ⎝ ⎠                                   CV ,m


TV γ −1 = constant
PV γ = constant
VT c = constant
T γ P 1−γ = constant
Conclusion of Ist Law of Thermodynamics

• The internal energy of an isolated system is a constant
  For isolated system : dU = 0; (as q = 0, w = 0» No perpetual
  motion machines! )

 • The energy of the universe is constant. ∆Usystem = −∆Usurroundings

 • When a system undergoes a process that leads to a change of
    state then the sum of the heat q transferred and the work w
    performed, is equal to the change in the internal energy dU of
    the system.
 dU = ∂q + ∂w (Closed system, through a number of steps)

 • A system contains ONLY internal energy. A system does not
    contain heat or work.
Conclusion of Ist Law of Thermodynamics


• Cyclic Process             ∫ dU   =0   (Exact differential)

• In a cyclic process the work done by a system on its
  surroundings is equal to the heat withdrawn from the
  surroundings .
                   - δ w = δq

• For an Adiabatic Process     δ wad = dU ; (as δq = 0)

• For a Non-Adiabatic Process
  δq = dU − δw ≡ δq = (δwad – δw); (as, δwad = dU)
Calculation of thermodynamic functions
                  for various processes

       reversible phase      const p heating, no   const V heating, no
     change at const. T, p      phase change          phase change


w     − ∫ p dV = − pΔV        − ∫ p dV = − pΔV        0

q      latent heat            q p = ΔH                 qV = ΔU

ΔU      q + w                 q + w                   = ∫ CV (T )dT

ΔH      q                     = ∫ C p (T )dT           ΔU + VΔp
Calculation of thermodynamic function for
             various processes for Ideal Gas


     Reversible, no phase change            rev, isothermal   rev, adiabatic
     rev        rev, const   irrev, const
                  ext. p        final p

w                                             − nRT ln
                                                       V2     = ∫ CV (T )dT
      − ∫ PdV    − pex ΔV − p f ΔV                     V1

q      ΔU-w                                   nRT ln
                                                       V2
                                                               0
                                                       V1
ΔU
      = ∫ CV (T )dT                            0              = ∫ CV (T )dT

ΔH
      = ∫ C p (T )dT                           0              = ∫ C p (T )dT
SUMMRAY OF ADIABATIC WORK (with solved example)


•    Reversible Adiabatic Expansion (or compression) of an Ideal Gas

                   1 mole gas (V1,T1) = 1 mole gas (V2,T2)

      adiabatic ⇒                đq = 0              Reversible ⇒                            đw = -pd V
                                 Ideal gas ⇒         dU = Cv d T

      ∴         From 1st Law           dU = -pd V ⇒                  CvdT = -pdV along path

                                       dT      dV
      CV dT = − pdV          ⇒    CV      = −R
                         p =RT         T       V
                            V
                                                                                                            Cp
                                                     R CV                                                        −1
          T2   dT       V dV               ⎛T2 ⎞ ⎛V1 ⎞                 C p −CV =R for i.g.       ⎛T2 ⎞ ⎛V1 ⎞CV
      CV ∫        = −R ∫
                         2
                                       ⇒   ⎜ ⎟=⎜ ⎟                   ⎯⎯⎯⎯⎯⎯→                     ⎜ ⎟=⎜ ⎟
          T1   T        V V
                         1
                                           ⎝T1 ⎠ ⎝V2 ⎠                                           ⎝T1 ⎠ ⎝V2 ⎠

                                                         γ −1

                           Cp              ⎛T2 ⎞ ⎛V1 ⎞
      Define           γ ≡         ⇒       ⎜ ⎟ =
⎜ ⎟
                           CV              ⎝T1 ⎠ ⎝V2 ⎠

                                                    3 ⎫

                                               CV = R ⎪
                                                   2 ⎪      5
    For monatomic ideal gas:                          ⎬ γ =    ( > 1 generally)

                                                   5 ⎪      3

                                               Cp = R
                                                   2 ⎪⎭


    In an adiabatic expansion (V2 > V1), the gas cools (T2 > T1).
    And in an adiabatic compression (V2 < V1), the gas heats up.

                                                                                         γ
                                                  pV                  ⎛ p2 ⎞ ⎛V1 ⎞
For an ideal gas (one mole)                   T =                ⇒    ⎜ ⎟=⎜ ⎟                  ⇒ pV1 γ = pV2γ
                                                   R                  ⎝ p1 ⎠ ⎝V2 ⎠
                                                                                                  1       2




                pV γ   is constant along a reversible adiabat



For an isothermal process                      T = constant                   ⇒              pV = constant
p
            p1                                        V2adiabat < V2isotherm
                                                      because the gas
                                                      cools during reversible
            p2                                        adiabatic expansion


                       V1          V2ad V2iso



•	 Irreversible Adiabatic Expansion of an ideal gas against a constant
   external pressure

                 1 mol gas (p1,T1) = 1 mol gas (p2,T2)                      (pext=p2)

     adiabatic                     ⇒      đq = 0 

     Constant pext = p2            ⇒      đw = -p2dV

     Ideal gas                     ⇒      dU = CvdT

     1st Law                       ⇒      dU = -p2dV


                   ∴        Cv d T = - p2 dV

     Integrating:           Cv ( T2 - T 1 ) = - p2 ( V2 - V1 )

                                                          ⎛         p2 ⎞

     Using pV = RT                        T2 (CV + R ) =T1 ⎜ CV +     R⎟
                                                          ⎝         p1 ⎠



     Note          p2 < p1         ⇒      T2 < T1        Again, expansion cools

     Note also (-wrev) > (-wirrev) 	             Less work is recovered through
                                                 an irreversible process
Some Thermodynamic Cycles
                                                                                                                 đq
•         Reversible	 Ideal Gas processes: Find ∆U , ∆H , q , w ,                                             ∫T

                                    (I	
                                      )                                                (II)
                 p                                                   p
                       (T )
                         1                                                 (T )
                                                                             1    D (const. p)   (T )
                                                                                                   3
                p1                                                p1
                                  A (isotherm)
                              B                 (T )                              A               E (const. V)
                p2                                1               p2
                p3            (rev.              C (const. V)                     (isotherm)     (T )
                                                                                                   1
                              adiabat)      (T )
                                              2


                            V1              V2
                              V1                 V2

                                                       const. T
          [A]    1 mol gas (p1,V1,T1)                    =           1 mol gas (p2,V2,T1)

          Ideal gas isotherm:                             ∆UA = 0                     ∆HA = 0 as, ΔH = Cp ΔT = 0

                                        V                           V                    đ qA            V2
                            wA = −RT1 ln 2               qA = RT1 ln 2                 ∫T       = R ln
                                        V1                          V1                                   V1

                                                       rev.adiabat
          [B]    1 mol gas (p1,V1,T1)                      =             1 mol gas (p3,V 2,T2)

          Adiabat:            	       qB = 0



                                      ∆UB = CV (T2 −T1 )

    Ideal gas:	
                                      ∆HB = C p (T2 −T1 )


    1st              Law:             w B = CV (T2 −T1 )	

                                          đqB
                                     ∫T          =0
reversible
  [C]          1 mol gas (p3,V2,T2)                 =           1 mol gas (p2,V2,T1)
                                                const. V



                                                                                 ∆UC = CV (T1 −T2 )
  Constant V:                  wC = 0                        Ideal gas:
                                                                                 ∆HC = C p (T1 −T2 )
  1st Law:                     qC = CV (T1 −T2 )


                                  đqC           ⎛T ⎞
                                 ∫T     = CV ln ⎜ 1 ⎟
                                                ⎝T2 ⎠



        [A]                    vs.               [B] + [C]

        ∆UA = 0                       ∆UB + ∆UC = 0 = ∆UA

        ∆HA = 0                       ∆HB + ∆HC = 0 = ∆HA


                 V
      qA = RT1 ln 2                       qB + qC = CV (T1 −T2 ) ≠ qA
                 V1
                   V
      w A = −RT1 ln 2                        wB + w C = CV (T2 −T1 ) ≠ w A
                   V1
         đqA        V2                        đqB           đqC          ⎛V ⎞     đq
        ∫T     = R ln                     ∫T        +∫            = R ln ⎜ 2 ⎟ = ∫ A
                    V1                                      T            ⎝V1 ⎠    T


                                ⎛ đq ⎞
      This result suggests that ⎜ ∫ rev ⎟ is a state function!
                                ⎝ T ⎠



               ∆UD = CV (T3 −T1 )
[D]                                              qD = C p (T 3 − 1
                                                               T         )
               ∆H D = C p(T 3−T 1)



                                                                  đqD            ⎛T ⎞
                         wD = −R (T3 −T1 )                      ∫T      = C p ln ⎜ 3 ⎟
                                                                                 ⎝T1 ⎠
∆UE = CV (T1 −T3 )
[E]                                          wE = 0          qE = CV (T1 −T3 )
             ∆HE = C p (T1 −T3 )

                đqE              ⎛T ⎞
               ∫T        = CV ln ⎜ 1 ⎟
                                 ⎝T3 ⎠




      [A]                       vs.                  [D] + [E]

      ∆UA = 0                            ∆UD + ∆UE = ∆UA
      ∆HA = 0                            ∆HD + ∆HE = ∆HA

                 V
      qA = RT1 ln 2                          qD + qE = R (T3 −T1 ) ≠ qA
                 V1
                   V
      w A = −RT1 ln 2                        wD + w E = −R (T3 −T1 ) ≠ w A
                   V1


       đqA          V2                đqD        đqE          ⎛V ⎞     đq
      ∫T     = R ln                ∫T       +∫         = R ln ⎜ 2 ⎟ = ∫ A
                    V1                           T            ⎝V1 ⎠    T


                        ⎛ đq ⎞
             Here again ⎜ ∫ rev ⎟ looks like a state function!
                        ⎝ T ⎠
Conclusion of Ist Law of Thermodynamics

• The internal energy of an isolated system is a constant
  For isolated system : dU = 0; (as q = 0, w = 0» No perpetual
  motion machines! )

 • The energy of the universe is constant. ∆Usystem = −∆Usurroundings

 • When a system undergoes a process that leads to a change of
    state then the sum of the heat q transferred and the work w
    performed, is equal to the change in the internal energy dU of
    the system.
 dU = ∂q + ∂w (Closed system, through a number of steps)

 • A system contains ONLY internal energy. A system does not
    contain heat or work.
Conclusion of Ist Law of Thermodynamics


• Cyclic Process             ∫ dU   =0   (Exact differential)

• In a cyclic process the work done by a system on its
  surroundings is equal to the heat withdrawn from the
  surroundings .
                   - δ w = δq

• For an Adiabatic Process     δ wad = dU ; (as δq = 0)

• For a Non-Adiabatic Process
  δq = dU − δw ≡ δq = (δwad – δw); (as, δwad = dU)
Calculation of thermodynamic functions
                  for various processes

       reversible phase      const p heating, no   const V heating, no
     change at const. T, p      phase change          phase change


w     − ∫ p dV = − pΔV        − ∫ p dV = − pΔV        0

q      latent heat            q p = ΔH                 qV = ΔU

ΔU      q + w                 q + w                   = ∫ CV (T )dT

ΔH      q                     = ∫ C p (T )dT           ΔU + VΔp
Calculation of thermodynamic function for
             various processes for Ideal Gas


     Reversible, no phase change            rev, isothermal   rev, adiabatic
     rev        rev, const   irrev, const
                  ext. p        final p

w                                             − nRT ln
                                                       V2     = ∫ CV (T )dT
      − ∫ PdV    − pex ΔV − p f ΔV                     V1

q      ΔU-w                                   nRT ln
                                                       V2
                                                               0
                                                       V1
ΔU
      = ∫ CV (T )dT                            0              = ∫ CV (T )dT

ΔH
      = ∫ C p (T )dT                           0              = ∫ C p (T )dT
Variation of U with system variables:

 U = f (V , T )           ⎛ ∂U ⎞
                     dU = ⎜
                                      ⎛ ∂U ⎞
                               ⎟ dV + ⎜     ⎟ dT
                          ⎝ ∂V ⎠T     ⎝ ∂ T ⎠V

1. Change in U w.r.t. T at constant volume
     ⎛ ∂U ⎞
Cv = ⎜    ⎟ ; qv = Cv ΔT = ΔU
     ⎝ ∂T ⎠ V
                                          ⎛ ∂U ⎞
2. Change in U w.r.t. V at constant temp: ⎜    ⎟
                                          ⎝ ∂V ⎠ T
 = π T dV + C V dT   For real gas
dU = CV dT (for ideal gas) As For ideal gas π T = ⎜
                                                          ⎛ ∂U ⎞
                                                               ⎟ =0
                                                          ⎝ ∂V ⎠T
3. Change in U w.r.t. T at constant pressure
             ⎛ ∂U ⎞
dU = Cv dT + ⎜    ⎟ dV  ⎛ ∂U ⎞          ⎛ ∂U ⎞
             ⎝ ∂V ⎠ T   ⎜ ⎟ = Cv + αV ⎜      ⎟
                             ⎝ ∂T ⎠ P          ⎝ ∂V ⎠ T
⎛ ∂U ⎞        ⎛ ∂U ⎞ ⎛ ∂ V ⎞
⎜    ⎟ = Cv + ⎜    ⎟ ⎜ ⎟
⎝ ∂T ⎠ P      ⎝ ∂V ⎠ T ⎝ ∂T ⎠ P where
Change in Internal Energy at Constant P

• Suppose we want to know how the internal energy, U, changes with
  temperature at constant pressure        dU = π dV + C dT
                                                   T        V


                                           ⎛ ∂U ⎞ ⎛ ∂ (π T dV + C V dT)⎞
                                           ⎜ ⎟ =⎜                      ⎟
                                           ⎝ ∂T ⎠ p ⎝       ∂T         ⎠p
                                           ⎛ ∂U ⎞         ⎛ ∂V ⎞
                                           ⎜ ⎟      = π T ⎜ ⎟ + CV
                                           ⎝ ∂T ⎠ p       ⎝ ∂T ⎠ p
   – But the change in volume with temperature at constant
     pressure is related to the Isobaric thermal expansion /
     expansion coefficient of the gas, α
                                              1 ⎛ ∂V ⎞        ⎛ ∂V ⎞
                                         α=     ⎜ ⎟        or ⎜ ⎟ = αV
                                              V ⎝ ∂T ⎠ p      ⎝ ∂T ⎠ p
                                            ⎛ ∂U ⎞
                                         so ⎜ ⎟ = π Tα V + C V
                                            ⎝ ∂T ⎠ p

       • Large α means sample responds strongly to changes in T
       • For an ideal gas, πT = 0 so
                                          ⎛ ∂U ⎞
                                          ⎜    ⎟ = CV [definition ]
                                          ⎝ ∂T ⎠ p
Variation of V with system variables: Experimentally known that the
Volume of an isotropic material is a function of Temperature and Pressure.




                                             isothermal compressibility




                      relative/fractional    coefficient of Isobaric
                      change of Volume       thermal expansion /
                                             expansion coefficient
For an ideal gas : PV = nRT

                       similarly κT = 1/p


                      For solid and liquid α and κT are approx.
                      independent of T & p
Another quantity of interest which can be obtained from α and κT is:


  This derivative tells us how fast the pressure rises when we try
  to keep the volume constant while increasing the temp.


 Exercise:
 How much pressure would be generated in a mercury thermometer if we tried to
 heat the thermometer higher than the temperature where the mercury has
 reached the top of the thermometer. Given: For Hg, α = 1.82 Ø 10×4 K×1 and κT
 = 3.87 Ø 10×5 atm×1
                            We see that each 1 C increases the pressure by
                            4.7 atm, about 69 lb/sq in. This is a lot of
                            pressure for a glass tube to withstand. It
                            wouldn't take very many degrees of temperature
                            increase to break the glass thermometer.!!!




     Using a variation of Euler's
     chain rule we can write
Variation of H with system variables: H = f ( P, T ) dH = ⎛ ∂H ⎞ dP+⎛ ∂H ⎞ dT
                                                          ⎜    ⎟    ⎜    ⎟
                                                          ⎝ ∂P ⎠T   ⎝ ∂T ⎠ P
1. Change in H w.r.t. T at constant pressure
      ⎛ ∂H ⎞
C p = ⎜ ⎟ ; q p = C p ΔT = ΔH
      ⎝ ∂T ⎠ P
                                                     ⎛ ∂H ⎞
 2. Change in H w.r.t. P at constant temperature: ⎜ ⎟⎝ ∂P ⎠ T
H = f ( P, T )
                                                 ⎛ ∂H ⎞
                                  Alternately, = ⎜     ⎟ dP + CP dT
⎛ ∂H ⎞ ⎛ ∂P ⎞ ⎛ ∂T ⎞                             ⎝ ∂P ⎠T
⎜ ⎟ ⎜ ⎟ ⎜ ⎟ = −1
⎝ ∂P ⎠ T ⎝ ∂T ⎠ H ⎝ ∂H ⎠ P
                              dH = Cp dT (for ideal gas)
  ⎛ ∂H ⎞   ⎛ ∂T ⎞ ⎛ ∂H ⎞
∴ ⎜ ⎟ = −⎜ ⎟ ⎜ ⎟ = − μ JT C p                 ∂H ⎞
  ⎝ ∂P ⎠ T ⎝ ∂P ⎠ H ⎝ ∂T ⎠ P  For ideal gas ⎛
                                            ⎜    ⎟ = 0
                                                          ⎝ ∂P ⎠T
3. Change in H w.r.t. T at constant volume: ⎛ ∂H ⎞
                                                    ⎜ ⎟
              ⎛ ∂H ⎞                                ⎝ ∂T ⎠ V
dH = C P dT + ⎜ ⎟ dP
              ⎝ ∂P ⎠ T
                                                      ⎛ ∂H ⎞           ⎛ ∂P⎞    α
⎛ ∂H ⎞        ⎛ ∂H ⎞ ⎛ ∂ P ⎞
                             From earlier results     ⎜ ⎟ = −μ JT Cp ; ⎜ ⎟ =
⎜ ⎟ = CP + ⎜ ⎟ ⎜ ⎟                                    ⎝ ∂P ⎠ T         ⎝ ∂T ⎠ V κ
⎝ ∂T ⎠ V   ⎝ ∂P ⎠ T ⎝ ∂T ⎠ V
                                                      ⎛ ∂H ⎞   ⎡ αμ ⎤
                                                     ∴⎜ ⎟ = CP ⎢1 − JT ⎥
                                                      ⎝ ∂T ⎠ V ⎣    κ ⎦
The Joule-Thomson Expansion Expt

The Joule-Thomson experiment consists of forcing a gas at constant
backing pressure passing through a porous plug under adiabatic condition
and measuring the change in temperature.

                                       ⎛ ∂T ⎞ ≈ ΔT
The Joule-Thomson coefficient (μJT ) = ⎜    ⎟
                                       ⎝ ∂P ⎠ H Δp

The most straightforward way to measure the coefficient is to measure
the temperature of the gas entering and leaving the porous plug and
divide the change in temperature by the
change in pressure:



we need to decide what is being held constant when we take the partial
derivative. In this case, since q =0, the change in internal energy of the
gas is equal to w.
Joule-Thompson Experiment: Inversion Temperature

                                  In this experiment q = 0
                                  w = - pf (Vf – 0) - pi (0 - Vi)

                                  ΔU = Uf – Ui = q + w = - pfVf + piVi
                                  Uf + pfVf = Ui + piVi
                                  Hf = Hi , ΔH = 0      Isenthalpic process

                                                        ⎛ ∂H ⎞         ⎛ ∂H ⎞
                                  H = f ( P, T ); dH = ⎜      ⎟ dP + ⎜      ⎟ dT
                                                        ⎝ ∂P ⎠T        ⎝ ∂T ⎠ P
                                           ⎛ ∂H ⎞      ⎛ ∂H ⎞ ⎛ ∂T ⎞
                                           ⎜
                                           ⎜ ∂p ⎟ ⎟ = −⎜    ⎟ ⎜ ⎟ = −C p × μ
                                                                ⎜ ⎟
   Applying Euler’s Chain Rule,   we get: ⎝       ⎠T   ⎝ ∂T ⎠ p ⎝ ∂p ⎠ H

Joule-Thompson Coefficient , μ (or μJT ) =      ⎛ ∂T ⎞ ≈ ΔT in this J-T expt.
                                                ⎜ ⎟
                                                ⎝ ∂P ⎠ H Δp
                     ⎛ ∂H ⎞      ⎛ ∂H ⎞
H = f ( P, T ); dH = ⎜    ⎟ dP + ⎜    ⎟ dT       dH = − μC p dP + C p dT
                     ⎝ ∂P ⎠T     ⎝ ∂T ⎠ P
THE JOULE-THOMPSON EXPERIMENT

   ⎛ ∂T ⎞
μ =⎜ ⎟
   ⎜ ∂p ⎟
   ⎝    ⎠H
If μ > 0 then this indicates that
the gas cools (-ve δT) when gas
expanded (-ve δp).

If μ < 0 then this indicates that
the gas heats (+ve δT) when
expanded (-ve δp).

The "inversion temperature"
indicates where on a (T, p)
isenthalpic plot the (dT/dP)H flips
from +ve to –ve. Or,point where µ
changes sign from + to –
ve and the point is the maximum
inversion temperature

For a real gas µ is non-zero
(except at the maximum inversion
temperature)
2




          ⎛ ∂T ⎞
    2

        μ=⎜
          ⎜    ⎟
          ⎝ ∂p ⎟ H
               ⎠




                     The Linde process
Joule-Thompson              ⎛ ∂T ⎞ ≈ ΔT
    Coefficient , μ (or μJT ) = ⎜ ∂P ⎟
                                ⎝ ⎠ H Δp
•   µ can be either (+) or (-)
     – Positive µ means dT is negative when
       dp is negative
        •Gas cools on expansion
     – Negative µ means that means dT is
       positive when dp is negative
        •Gas warms on expansion
     – Transition between positive and
       negative µ is called the Joule-
       Thompson inversion temperature
        •Gases have both high and low
        inversion temperatures
     – Ideal gas µ = 0, T unchanged by                Tinversion       µ
       change in p on expansion                Gas       (K)       (K atm-1)
                                              CO2    1500          1.11
•   Practical applications:                   N2     621           0.25
     – Gas liquefaction                       He     621           0.25
     – Isotope separation
⎛ ∂T ⎞    T ( ∂V ∂ T   )P   −V
μJT   =⎜     ⎟ =
       ⎝ ∂ P ⎠H         CP
⎛ ∂T ⎞    T ( ∂V ∂ T   )P   −V
μJT   =⎜     ⎟ =
       ⎝ ∂ P ⎠H         CP
For a van der Waal gas:
                                           Therefore, μJT depends critically on
         ⎛ ∂T ⎞     T ( ∂V ∂ T )P − V
 μJT    =⎜     ⎟  =                        the constants a and b, which are the
         ⎝ ∂ P ⎠H          CP
                                           indices of non zero interaction and
 μJT =
          1    ⎛ 2a    ⎞
                    − b⎟                   finite volume of the gas molecules
               ⎜
          CP   ⎝ RT    ⎠

      2a
 If ,    > b then μ > 0 (cooling observed )
      RT                                           • If initial Temp (Ti) is below
      2a                                             Tinversion only then cooling is
 If ,    < b then μ < 0 ( heating observed )
      RT                                             observed.
 Inversion temperature                             • And the final temp T2 is
μ JT = 0 when         T = Tinversion                 lower than T1

          1    ⎡ 2a    ⎤         ⎛ 2a ⎞
∴ 0=           ⎢    − b⎥    or , ⎜
                                 ⎜ RT        ⎟=b
                                             ⎟
          Cp   ⎣ RT    ⎦         ⎝ inversion ⎠
                 2a
∴ Tinversion =
                 Rb
N2 and O2 will cool upon expansion at
room temperature, but He and Ne will
warm upon expansion at room
temperature.
Derive the Following expressions

                      For ideal gas
⎛ ∂P ⎞ α                                          1 ⎛ ∂H ⎞
⎜    ⎟ =                              ∴μ JT   =−     ⎜    ⎟
⎝ ∂T ⎠V κ                                        C p ⎝ ∂P ⎠ T
                                             ⎛ ∂T ⎞    T ( ∂V ∂ T   )P   −V
           α TV
            2
                                      μJT   =⎜     ⎟ =
C p − CV =                                   ⎝ ∂ P ⎠H         CP
            κ                         for ideal    gases :    μJT = 0

                                              1 ⎛ 2a      ⎞
                                      μJT =            − b⎟
                                              C P ⎜ RT
                                                  ⎝       ⎠



                                            ⎛ ∂H ⎞
Isothermal Joule-Thompson Coefficient, μT = ⎜    ⎟ μT = - Cpμ
                                            ⎝ ∂P ⎠T
Monoatomic ideal gas CV,m = 3R/2, Cp,m = 5R/2
The Perfect gas and πT, α, κT, μ

Property             PD                Value for Perfect Gas          Info:

Internal               ⎛ ∂U ⎞
Pressure          πT = ⎜    ⎟
                         ∂V ⎠T
                                               πT=0            Strength/nature of
                       ⎝                                       interactions between
                                                               molecules


 Expansion          1 ⎛ ∂V ⎞                  α =1 / T
                                                                The higher T, the less
 Coefficient      α= ⎜ ⎟                                        responsive is its volume
                    V ⎝ ∂T ⎠ p                                  to a change in
                                                                temperature

                           1 ⎛ ∂V ⎞
Isothermal        κT = −
                           V⎝
                             ⎜
                             ⎜ ∂p ⎟
                                  ⎟           κT=1 / p          The higher the p, the
Compressibility                   ⎠T                            lower its compressibility




                       ⎛ ∂T ⎞
Joule-Thomson
                    μ =⎜
                       ⎜    ⎟
                            ⎟                   μ=0            Another indication of
Coefficient            ⎝ ∂p ⎠ H                                molecular interactions.
Ist Law of Thermodynamics:
• The different forms of energy are inter convertible.
• When one form of energy disappears an equivalent of another kind
    must appear. Conversion of energy.
•   Energy can be transferred / transformed, keeping the total energy
    fixed.
             qsys = - qsurr     ΔU = q + w (= – pexdV)
             wsys = - wsurr     ∆U = q – pexdV


Incompleteness of Ist Law: It Does not say anything about:

• Whether any transfer / transformation of energy would occur     at all?
• If it does, then in which direction would the change occur?
• If any transfer / transformation of energy occurs in a particular
    direction, then how long will it be sustained?
•   If any transfer / transformation of energy occurs in a particular
    direction, then how fast will it proceed?
What happens when ?              Free Expansion of Gas

                             Gas                  Gas



                              Valve                           Gas
                                       Vacuum       Valve
                              Closed
                                                    Open
  Gas 1            Gas 2
                            Gases tend to occupy the whole available
Ideal gas mixture ΔH=0      volume of the container.
Two questions:
1) Does the enthalpy of the system increase or decrease and how
much ?
2) Does the system become more or less disordered and by how
much?
The driving force of such a process is the increase of the disorder
in the system.
Warm
Thermal Conduction




                                   The two liquids (with very similar molecules) form
                                   an ideal solution (ΔH ≈ 0), in which the molecules
                                   are randomly and uniformly mixed.
                     Hot dQ Cold




                                   Suppose two bodies are brought in contact. Then
                                   from the Ist law, we ONLY know if q heat was lost
                                   by one, exactly q heat would be gained by the other.
                                   The law does not specify if the Ist one will lose heat
                                   or, the other one. To know the direction of flow of
                                   heat, we need another information, namely the
                                   temp of the two bodies.
First Law of Thermodynamics


• Conservation of Energy
• Says Nothing About Direction of Energy Transfer


            Second Law of Thermodynamics
 • Preferred (or Natural) Direction of Energy Transfer
 • Determines Whether a Process Can Occur


 • Thermodynamic Processes can be classified into Three Types :
    – Natural (or Irreversible)
    – Impossible
    – Reversible
Disorder increase for the following processes:
• Solids melt to liquids
• Solids or liquids vaporize to form gases
• Solids or liquids dissolve in a solvent to form non-electrolyte
solution
• A substance is heated (increased temperature increases the
molecular motions and the disorder)
• A chemical reaction produces an increase in the number of
molecules of gases

• The 2   Law puts forward the criteria for the direction of the
         nd

spontaneous chemical/ physical change of a thermodynamic system.

• The historical roots of the second law stems from the invention of
heat engine (namely, the steam engine). It is known that work can
be fully converted to heat (joule’s expt), the question is can heat
be converted to work???
Entropy
• The thermodynamic property of a system that is related to its
  degree of randomness or disorder is called entropy (S).

• The entropy S and the entropy change ΔS=S2-S1 are state
  functions

• The entropy S has a unique value, once the pressure P, the
  temperature T and the composition n of the system are specified,
  S = S (p,T,n)

• The entropy is an extensive property, i.e. increases with the
  amount of matter in the system.
Carnot Engine: Introduction to Heat Engines

   •   One of the primary applications of
       thermodynamics is to Turn heat into work

   •   The standard heat engine works on a
       reversible cyclic process:
            1. extract heat from a hot reservoir,
            2. perform work,
            3. dump excess heat into a cold
          reservoir (often the environment).

   A “reservoir” is a large body whose
   temperature doesn’t change when it absorbs
   or gives up heat

Carnot and then by Clausius: Statement of the Second law :
It states that it is impossible to construct a device that operates in
a cycle and produces no effect other than the transfer of heat from
a lower-temperature body to a higher-temperature body.
TH
                TH


                    QH                                      QH


                                                        R         WOUT
                HE            WOUT

                     QL                                      QL

                                                        TL
                TL



                                     −W
Thermal efficiency = ε =
                                     QH
For a complete cycle: dU = 0

 ∴         Qcy = - Wcy

Qcy = QH - Qc
               −W            QH − Qc
∴ε   cyc   =
               QH
                         =
                               QH
                                         Q
                                     = 1− c
                                         QH

The engine will have 100% efficiency only when Qc = 0
Heat Engines


• By conservation of energy:
                 |QH| = |W| + |QL|.
• The high and low temperatures TH and TL are called
  the operating temperatures of the engine.

• We will considering only engines that run in a
  repeating cycle, that is, the system returns
  repeatedly to its starting point, and thus can run
  continuously.

• Absolute value signs are used because we are
  interested only in the magnitudes.
Second Law of Thermodynamics.
                   The Carnot Cycle.

• The Carnot cycle is an
  example of a reversible
  process, which is a process
  that can be done in
  reverse.

• A reversible process
  requires that any changes
  are made infinitely slowly.

• Real processes are not
  reversible due to friction ,
  turbulence in the gas, etc.
Second Law of Thermodynamics: The Carnot Cycle
•    Four steps
•    Isothermal expansion: a to b
•    Adiabatic expansion: b to c
•    Isothermal compression: c to d
•    Adiabatic compression: d to a


      Define the efficiency ε

          work done by system         " work"
ε ≡                                 =
       heat extracted from reservoir " cost"
                                                Valid for all heat engines.
                     W                  QC
    efficiency = ε =    = 1−                    (∆U = 0 for closed cycle)
                     QH      QH
    where, W = │QH│ - │Qc│; following conservation of energy
The Carnot Cycle


• Step 1: a to b.

   – The gas is in contact with a
     heat bath at temperature TH
     and weight is removed from
     the piston.

   – The gas expands, while
     maintaining a constant
                                                   Vb
     temperature, isothermal        w1 = − nRTH ln
                                                   Va
   – the change in the internal
     energy is thus equal to zero   dU = 0
                                    w1 = − q1
The Carnot Cycle

• Step 2: b to c.

   – The gas is isolated from
     the environment and some
     more weight is removed
     from the piston.

   – The gas expands and during
     the adiabatic expansion, the
     temperature of the gas will
     decrease.
                                            γ −1            γ −1
                                    TH Vb          = TLVc
   – For adiabatic expansion pVγ
     is constant, and we can        w2 = nCV (TL − TH )
     thus related state b to
     state c:
                                    q2 = 0
The Carnot Cycle


• Step 3: c to d.

   – The gas is in contact with
     a heat bath at
     temperature TC and weight
     is added to the piston.

   – The gas is compressed,
     while maintaining a constant                  Vd
     temperature, isothermal        w3 = − nRTL ln
                                                   Vc
   – the change in the internal
     energy is thus equal to        dU = 0
     zero
                                    w3 = − q3
The Carnot Cycle


• Step 4: d to a.

   – The gas is isolated from the
     environment and some more
     weight is added to the piston.

   – The gas is compressed and
     during the adiabatic
     compression, the temperature
     of the gas will increase.
                                              γ −1            γ −1
                                      TH Va          = TLVd
                                      w4 = nCV (TH − TC )
                                      q4 = 0
Vb
• Four steps                       w1 = − nRTH ln
• Isothermal expansion: a to b                    Va
                                   dU = 0
                                   w1 = − q1
                                           γ −1            γ −1
• Adiabatic expansion: b to c      TH Vb          = TLVc
                                   w2 = nCV (TL − TH )
                                   q2 = 0
                                                 Vd
• Isothermal compression: c to d   w3 = −nRTL ln
                                                 Vc
                                   dU = 0
                                   w3 = −q3
• Adiabatic compression: d to a            γ −1            γ −1
                                   TH Va          = TLVd
                                   w4 = nCV (TH − TC )
                                   q4 = 0
wcycle = w1 + w2 + w3 + w4

                     Vb                            V
wcycle = − nRTH ln      + nC v (TL − TH ) − nRTL ln d + nC v (TH − TL )
                     Va                            Vc
                     Vb          V
wcycle = − nRTH ln      − nRTL ln d
                     Va          Vc

∫ dU = 0
                  Vb         Vd TH Vb γ −1 = TLVc γ −1
qcycle   = nRTH ln + nRTH ln
                  Va         Vc TLVd γ −1 = TH Va γ −1
                                              γ −1   γ −1
                                      TH Vc     Vd            Vc   Vd
wcycle
                  V           V
         = nRTH ln a − nRTL ln d        = γ −1 = γ −1       ∴    =
                                      TL Vb     Va            Vb   Va
                  Vb          Vc
                           Va
wcycle   = nR(TH − TL ) ln
                           Vb
W       QC
efficiency = ε =    = 1−
                 QH      QH
But, QH = q1 = -w1   And, Qc = q3 = -w3
              Vb                   Vd TH Vb γ −1 = TLVc γ −1
w1 = −nRTH ln        w3 = −nRTL ln
              Va                   Vc T V γ −1 = T V γ −1
                                       L d            H a
dU = 0               dU = 0           TH Vc
                                                 γ −1
                                                        Vd
                                                           γ −1
                                                                                   Vc   Vd
                                                 =               =               ∴    =
w1 = −q1             w3 = −q3               TL       Vb
                                                          γ −1
                                                                     Va
                                                                          γ −1
                                                                                   Vb   Va

ε = 1 – │Qc│/ │QH│ = 1 – TLln (Vd/Vc)/ THln (Vb/Va)

   1 – │Qc│/ │QH│ = 1 – TL/ TH

  │Qc│/ │QH│ = TL/ TH            │Qc│/ │ TL │ = │QH│ / TH

  │Qc│/ │ TL │ – │QH│ / TH = 0 (here, Qc ≡ QL)

 qi    ∂q
∑ =0 ⇒∫ =0                      Thus, the term δq/T is a state function
 Ti    T
Carnot’s theorem tells us that no real engine can have an efficiency more
than that of the Carnot engine.

                    TH − TL     T
               η=           = 1− L
                      TH        TH
                    qH − qL
               η=
                      qH
                 qH − qL TH − TL
               ∴        =
                   qH      TH
                  qL      TL    qL TL
               1−    = 1−    ⇒−   +   =0
                  qH      TH    qH TH
               Multiply by qH TL
                qL qH      qH qL               q
               − +    = 0;   =               ⇒   = cons tan t
                TL TH      TH TL               T
When the Carnot cycle is operating as a heat engine (going
     around clockwise), w < 0, so that -w > 0 and q > 0.

                                          Va
                 wcycle = nR(TH − TL ) ln
                                          Vb
                                          − wcycle       wcycle
                 Efficiency, ε or η =                =
                                               q1         q1
                                          Va
                      − nR(TH − TL ) ln
                                          Vb     TH − TL      TL
                 η=                            =         = 1−
                                    Vb             TH         TH
                          nRTH ln
                                    Va
•    Efficiency of Carnot engine < 1
•    No cycle can have an efficiency greater than a Carnot cycle
•    All reversible engines operates between same 2 temperatures have same
    efficiency
Carnot Cycle (Ideal gas, All the steps are reversible)
                   1 (A to B)            2 (B to C)        3 (C to D)           4 (D to A)            Total (A to A)

  W           - nRThln(VB/V
                          A)             CV(T-T )
                                             C h      - nRT ln(VD/V
                                                          C       C)            CV(T-T )
                                                                                    h C        + nR(T – T) ln(V/V )
                                                                                                     C   h    B A


   q          + nRT ln(V/V )
                  h    B A                 Zero       + nRT ln(V/V )
                                                          C    D C               Zero         + nR h – T) ln(V/V )
                                                                                                  (T C       B A

  DU                     Zero            CV(T-T )
                                             C h                Zero            CV(T-T )
                                                                                    h C                     Zero



               + nR ln(V A)
                       B/V                 Zero          + nR ln(V C)
                                                                 D/V             Zero                       Zero
(qrev/ T)

                                                                                                          A (pA, VA, Th)


                                                                                                                       B (pB, VB, Th)
       γ −1                              γ −1            γ −1          γ −1            γ −1
TV            = const.; ThVB                    = TCVC          ThVA          = TCVD               (pD, VD, TC) D

                                                                                                                           C (pC, VC, TC)
                  γ −1            γ −1
         ⎛ VB ⎞           ⎛V ⎞             ⎛ VB ⎞ ⎛ VC ⎞
         ⎜ ⎟
         ⎜V ⎟            =⎜ C ⎟
                          ⎜V ⎟             ⎜ ⎟ =⎜ ⎟
                                           ⎜V ⎟ ⎜V ⎟                                                            Th > Tc
         ⎝ A⎠             ⎝ D⎠             ⎝ A⎠ ⎝ D⎠             ln (VD / VC ) = − ln (VB / VA )
Entropy

•   Our study of the Carnot cycle showed that
    over the cycle q/T = 0.

•   Since any reversible cycle can be
    approximated by a series of Carnot cycles, we
    expect that the integral of dQ/T along the
    closed path of the cycle = 0.

•   One consequence is that the integral of dQ/T
    between a and b is independent of the path.

•   The quantity dQ/T is called the entropy dS.

•   The entropy difference between a and b is
    thus path independent, and entropy is a state
    variable.
Entropy

•   Entropy is a state variable, but Q and W
    are not state variables since they depend
    on the path used to get from a to b.

•   For a reversible process, the change in
    the entropy of the engine is opposite to
    the change in entropy of the
    environment that provides the heat
    required (or absorbs the heat
    generated). The net change in the total
    entropy = 0.

•   For an irreversible process, the net
    change in the total entropy will be
    larger than 0.
Entropy :
  – Is a measure of the disorderness of a system.
  – In a reversible thermodynamic process, entropy of a system
    is related the change in the extent to which energy is
    dispersed in a disorderly manner, which in turn depends on
    the amount of energy transferred as heat (as heat
    stimulates motion) to the surroundings.
  – Is a measure of the energy in a system or process that is
    unavailable to do work.
  • For a process occurring at constant temperature (an
    isothermal process):



     qrev = the heat that is transferred when the process
     is carried out reversibly at a constant temperature.
     T = temperature at which the heat is transferred (in
     Kelvin).
Second Law of Thermodynamics

Entropy of the universe (i.e., Total Entropy):

• Does not change for reversible processes
• Increases for spontaneous processes.
• But, entropy can decrease for individual systems
 Reversible (ideal):


 Irreversible (real, spontaneous):
2nd law of thermodynamics

dSUniv = dSsys + dSsurr > 0        Spontaneous process
dSUniv = dSsys + dSsurr = 0        Equilibrium process
dSUniv = dSsys + dSsurr < 0        Impossible process

For any process
                      “=“ for reversible, equilibrium
dSsys + dSsurr ≥ 0    “>” spontaneous (irreversible) (real)
                        all spontaneous processes are irreversible
Example
 • Show the Carnot cycle on a T-S diagram and identify the heat
   transfer at both the high and low temperatures, and the work
   output from the cycle.


                             • 1-2, reversible isothermal heat transfer
T       1           2        QH = ∫TdS = TH(S2-S1) area 1-2-B-A
TH
                             • 2-3, reversible, adiabatic expansion
                             isentropic process, S=constant (S2=S3)
TL
            4        3
                             • 3-4, reversible isothermal heat transfer
                              QL = ∫TdS = TL(S4-S3), area 3-4-A-B
      A              B
       S1=S4       S2=S3 S • 4-1, reversible, adiabatic compression
                             isentropic process, S1=S4


 • Net work Wnet = QH - QL, the area enclosed by 1-2-3-4, the shaded
 area
Efficiency of an heat engine

                                                        TH
Consider a Carnot heat engine.
1.What fraction of the total heat transferred Qh
                                                             Qh
  to engine is converted into work in the cycle?
                                                                    Wby
                                                             QC
a. ∆T/TH           b. ∆T/TC             c. TC/TH
                                                             TC


2. What is efficiency of reverse engine (refrigerator)? Coefficient of
   Performance
a. QC / W           b. Tc/ (TH-TC)               c. 1-TH/TC



3. When can the heat engine convert the absorbed heat into work
  completely?.
a. At TH = -273 ˚C   b. At Tc = O ˚C        c. when TC =-273 ˚C
A Carnot heat engine receives 500 kJ of heat per cycle from a high-
 temperature heat reservoir at 652oC and rejects heat to a low-
 temperature heat reservoir at 30oC. Determine
 (a) The thermal efficiency of this Carnot engine.
 (b) The amount of heat rejected to the low-temperature heat reservoir.


a.                  TL
      η th , rev = 1 −
                    TH                             TH = 652oC
                     ( 30 + 273) K
               = 1−
                    ( 652 + 273) K                          QH

               = 0.672 or 67.2%                                     WOUT
                                                       HE

                                                               QL
       QL    T
b.         = L                                     TL = 30oC
       QH TH
              ( 30 + 273) K
           =                 = 0.328
             ( 652 + 273) K
       Q L = 500 kJ ( 0.328)
             = 164 kJ
Suppose a mole of a diatomic gas, such as O2, is compressed adiabatically so
the final volume is half the initial volume. The starting state is V = 1 liter,
T = 300 K. What are the final temperature and pressure?


                                                           p iV i γ = p f V fγ
Equation relating p,V for adiabatic process in α-
ideal gas                                                      γ =
                                                                      7/2
                                                                          = 1 .4
γ is the ratio of Cp/CV for diatomic gas in this case                 5/2
                                                                                     γ
                                                                        ⎛V       ⎞
Solve for pf from first equation                              pf   = pi ⎜ i      ⎟
                                                                        ⎜V       ⎟
                                                                        ⎝ f      ⎠
                                                                                          γ
Substitute for pi                                                    nRT i ⎛ V i
                                                                             ⎜
                                                                                         ⎞
                                                                                         ⎟
                                                                   =
                                                                       Vi ⎜ V f
                                                                             ⎝
                                                                                         ⎟
                                                                                         ⎠
                                                                   = 6 . 57 x10 6        Pa
                                                                       p fV f
Use ideal gas law to calculate final temperature              Tf =
                                                                      nR
OR use the equation relating T,V for an adiabatic                  = 395 K
process to get the final temperature (α = 5/2 for         T i α V i = T fα V f
diatomic gas)                                                                        1
                                                                       ⎛V        ⎞   α
                                                              T f = Ti ⎜ i       ⎟
Solve for Tf                                                           ⎜V        ⎟
                                                                       ⎝ f       ⎠
                                                                  = 395 K
Entropy change in heat engine

                                                          Th
Consider a Carnot heat engine.
1. What is the sign of the entropy change of                   Q
   the hot reservoir during one cycle?                               Wby
                                                               h
a. ΔSh < 0         b. ΔSh = 0       c. ΔSh > 0                 QC

Because energy is flowing out of the hot reservoir, its        Tc
entropy (the number of microstates) is decreasing.
2. What is the sign of the entropy change of the cold reservoir?
a. ΔSc < 0         b. ΔSc = 0         c. ΔSc > 0
Because energy is flowing into the cold reservoir, it’s entropy (number
of microstates) is increasing.

3. Compare the magnitudes of the two changes.
a. |ΔSc| < |ΔSh|   b. |ΔSc| = |ΔSh|        c. |ΔSc| > |ΔSh|
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Thermodynamics spring 2013

  • 1. CY 11001 CHEMISTRY Professor: Dr. Amita (Pathak) Mahanty Office: Room C-301 (2nd Floor, Chemistry Department) e-mail: ami@chem.iitkgp.ernet.in phone: 83312 (office) Ground Rules for the Class • Mobile Phones in switched off mode • Attendance is a must and will be checked regularly • Vast syllabus and fast paced, advised to take class notes
  • 2. SCHEDULE CHEMISTRY THEORY COURSE SECTIONS 1, 2 & 3 Physical: 3rd Jan, 2013 – 1st Feb, 2013 (11 lectures) Inorganic: 7th February, 2013- 15th March, 2013 (12 lectures) MID TERM SEMESTER EXAM … 18.02.2013 - 26.02.2013 (Monday -Tuesday) Organic: 18th March, 2013 - 12th April, 2013 (12 classes) Room No. Day Time Monday 4:30-5:25 F-116 Thursday 4:30-5:25 Lecture Timings: Friday 4:30-5:25
  • 3. Tutorial Schedule for Spring 2012-13 Sec & Tutorial Tutorial Tutorial Roll No Group Room Day Timings No (AM) Sec: 11A S-126 Thursday 10:30-11.25 AE, AG, BT, CE, CH, CS, CY Sec: 11B S-127 Thursday 10:30-11.25 EC, EE, EX, GG, HS, IE, IM, MA, ME10008 Sec: 11C F-131 Thursday 10:30-11.25 ME10022, MF, MI, MT, NA, PH, QD Sec: 12A S-126 Monday 8.30 - 9.25 AE, AG, BT, CE, CH, CS, CY20010 Sec: 12B S-127 Monday 8.30 - 9.25 CY20024, EC, EE, EX, GG, HS, IE, IM, MA20032 Sec: 12C F-131 Monday 8.30 - 9.25 MA20046, ME, MF, MI, MT, NA, PH, QD
  • 4. CY 11001 CHEMISTRY Distribution of Marks: Mid Semester Exam (Only Physical): 30% End Semester Exam (Inorganic & Organic): 50% Teachers Assessment (TA): 20% Break up: [Physical (6%), Inorganic (7%), Organic (7%)] TA marks to be based on a CLASS-TEST: 30th January 2013 Text Book: Atkin’s Physical Chemistry 8th Ed Reference Books: Physical Chemistry by Silbey, Alberty & Bawendy; Wiley. Physical Chemistry by I. N. Levine; McGrew. Physical Chemistry David W. Ball; Thompson.
  • 5. CY 11001 CHEMISTRY (L-T-P : 3-1-0; Credit : 4) Thermodynamics of Chemical Processes: • Review of Essential Concepts and Definitions • Revision: Heat, Work & Energy; First Law of Thermodynamics • The Second Law of Thermodynamics • Concept of Entropy • Gibbs Free Energy • Equilibrium conditions for Closed Systems • Maxwell Relations • The Chemical Potential • Definition and Concept of Open Systems • Phase and Reaction Equilibria Electrochemical Systems: • Electrochemical Cells and EMF • Applications of EMF Measurements: Thermodynamic data, Activity Coefficients, Solubility product and pH Kinetics of Chemical Reactions: • Reversible, Consecutive and Parallel Reactions, • Steady State Approximation, • Chain Reactions, Photochemical Kinetics
  • 6. Thermodynamic Thermodynamics provides a framework of relating the macroscopic properties of a system to one another. Thermodynamic: ↔ Classical, Statistical and Irreversible Classical Thermodynamics, to the study of macroscopic properties of system/matter at equilibrium using the laws governing transformation of energy from one form to another. It is concerned only with macroscopic quantities and ignores the microscopic variables that characterize individual molecules. THE BASIC CONCEPTS: System, the part of the world in which we have a special interest. Surroundings, the region outside the system where we make our measurements. Boundary, a hypothetical/real barrier between system and surroundings.
  • 7. Thermodynamic Systems Open systems can exchange both matter and energy with the environment. Closed systems exchange energy but not matter with the environment. Isolated systems can exchange neither energy nor matter with the environment.
  • 8. Thermodynamic Systems System : Open, Closed, Isolated Surroundings Boundary / Wall • Rigid and Non rigid (movable) • Permeable and Impermeable (no matter is allowed to pass through it) • Adiabatic and Diathermic boundary ( - permits the passage of energy as heat ) A system surrounded by a rigid, impermeable, adiabatic wall – Isolated system Example: Universe as a whole, a thermo flask
  • 9. Thermodynamic Equilibrium For Isolated system: • Macroscopic properties do not change with time For Non isolated system: a) Macroscopic properties do not change with time b) Removal of the system from contact with its surroundings causes no change in the properties of the system • A system in thermodynamic equilibrium is an equilibrium system • Thermodynamic State only defined by the present values of the state variables, not by the history What are conditions of Thermodynamic Equilibrium?
  • 10. Mechanical equilibrium The condition of equality of pressure on either side of a movable wall / boundary. No unbalanced forces act on or within the system – does not undergo acceleration or no turbulence inside the system
  • 11. Thermal equilibrium Thermal equilibrium between system and the surroundings, is a condition in which there is no change in the properties of the system or surroundings when they are separated by a thermally conducting wall. In other words, Thermal Equilibrium is a condition in which no change of state occurs when two objects A to B are in contact through a diathermic boundary.
  • 12. Material Equilibrium Concentrations of the chemical species in the various parts of the system are constant with time a) No net chemical reactions are occurring in the system b) There is no net transfer of matter from one part (phase) of the system to another or between the system and its surroundings Phase: a homogeneous part of a system is called a phase For thermodynamic equilibrium, all three kinds of equilibrium must be present No matter what is the initial state of an isolated system, eventually it will reach the state of thermodynamic equilibrium
  • 13. How do we define a system? State of a System Macroscopic state of a system can be specified by the values of a small number of macroscopic Properties/Parameters/Physical characteristics or attributes of a system - Thermodynamic variables Thermodynamic variables which are experimentally measurable • Composition – mass of each chemical species that is present in each phases, • pressure (P), volume (V), Temperature (T), density, etc. • field strength, if magnetic/electrical field act on the system • gravitational field (N.B.: only the average values are considered, all fluctuation and perturbations are ignored). On the other hand, Microscopic state of a system needs description of each molecule – a very complicated picture
  • 14. Thermodynamic State If the value of every thermodynamic property in system A is same as in system B – then they are in the same thermodynamic state The state of a thermodynamic system is defined by specifying the values of its thermodynamic properties – However, it is not necessary to specify all the properties to define the state of a system. In fact, the macroscopic state of a system can be specified by the values of a small number of macroscopic variables – these called the Properties / Parameters / Thermodynamic variables of a system. For instance: The thermodynamic state of a single-phase system of fixed amounts of non reacting substances can be described by any two of the three state functions (P, V and T) Equation of state, an equation that interrelates pressure, volume, temperature, and amount of substance: P = f (T, V, n).
  • 15. The Equation of State of Ideal Gases An equation of state - an equation that relates macroscopic variables (e.g., P, V, and T) for a given substance in thermodynamic equilibrium. In equilibrium (≡ No macroscopic motion), just a few macroscopic parameters are required to describe the state of a system. Geometrical representation of the equation of state: f (P,V,T) = 0 The ideal gas equation of state: PV = nRT an equilibrium P state P – pressure [Newtons/m2] V – volume [m3] the equation- n – number of moles of gas of-state surface T – the temperature in Kelvins [K] J R – a universal constant R ≈ 8.31 V mol ⋅ K T
  • 16. Recap The gas laws Boyle’s law: At constant temperature, the pressure of a sample of gas is inversely proportional to its volume, p ∝ 1/V at constant temperature. Charles’ law: At constant pressure, the volume of a gas is proportional to the absolute tem perature, V ∝ T at constant pressure. Avogadro’s principle: Equal volumes of gases at the same pressure and temperature contain the same numbers of molecules. Dalton’s law: The pressure exerted by a mixture of gases is the sum of the partial pressures of the gases.
  • 17. Thermodynamic Systems Homogeneous system, a system having its properties uniform throughout – a single phase solution / pure. Heterogeneous system, a system with more than one phase. Intensive properties Does not depend upon size (the quantity/amount of matter present) of the system [e.g. Pressure, Temp, Viscosity, Density etc.] Total Property = property of part of the system Extensive properties Depends upon size of the system [e.g. n, V, surface area etc ] Extensive properties depend on the amount of substance in the system.] Total Property = Σ property (in each part of the system) Other variables: Compositions, Surface area, Electrical/magnetic strength Gravitational field can/are generally ignored
  • 18. A very important macroscopic parameter: Temperature Temperature is a property associated with random motion of many particles. Introduction of the concept of temperature in thermodynamics is based on the the 0’th law of thermodynamics: B acts as Thermometer. A, B, C all are at the same “temperature”. A well-defined quantity called Temperature exists such that two systems will be in thermal equilibrium if and only if both have the same temperature.
  • 20. Thermodynamic State Variables / Properties Therefore, For describing the State of a System we require: • A few experimentally measureable macroscopic properties: p, T, V, n, m, ... • Knowledge if System is Homogeneous or Heterogeneous • Knowledge if System is in Equilibrium State • Knowledge of the number of components
  • 21. Thermodynamic Process: Operation for Change in State Change of State: Transformation e.g., 3 H2 (g, 5 bar, 100 °C) → 3 H2 (g, 1 bar, 50 °C) (initial state) (final state) Path: Sequence of Intermediate states through which a system passes to attain the final state Process: Operation through which a system undergoes a change in state. Process describes the path. Path Path can be: Reversible (always in Equilibrium) Irreversible (describes direction of time) Cyclic(initial and final state have the same value) Processes can be: • Adiabatic (No heat transfer between system and surrounding) • Isobaric (Constant pressure process) • Isothermal (Constant temp process) • Constant Volume process • Endothermic & Exothermic process (q<0 & q>0)
  • 22. Essential concepts / Definitions Processes : When one or more of the parameters of a system changes, the state of the system also changes and the system is said to have undergone a process. Various types of processes: • Isothermal (T), • Isobaric (P), • Isochoric (V) • Adiabatic (q), • Isenthalpic (H) • Exothermic & Endothermic • Cyclic Each process can be either carried out Reversibly or Irreversibly
  • 23. Thermodynamic Processes can be : Reversible process: Ideal process • Change must occur in successive stages of infinitesimal quantities • Infinite duration • Virtual thermodynamic equilibrium, at each of the small stages. • Changes of the thermodynamic quantities in the different stages will be the same as in the forward direction but opposite in sign w.r.t. forward direction. The system and surroundings can be put back in their original states by exactly reversing the process. Irreversible Process: Real / Spontaneous • Occurs suddenly or spontaneously without the restriction of occurring in successive stages of infinitetesimal quantities. Irreversible processes cannot be undone by exactly reversing the change to the system. • Do not remain in the virtual equilibrium during the transition. • The work (w) in the forward and backward processes would be unequal. Cyclic process: • Is one in which the initial and final states are the same. In such process: • There is no change in the state variables (e.g., ∫dU = Uf-Ui = 0) • In contrast, path functions generally have non-zero values for cyclic processes, dependent on the path (e.g., ∫δw ≠ (wf – wi) ≠ 0]
  • 24. Spontaneous Processes • Spontaneous processes are those that can proceed without any outside intervention. • The gas in vessel B will spontaneously effuse into vessel A, but once the gas is in both vessels, it will not spontaneously go back to B
  • 25. Reversible Processes In a reversible process the system changes in such a way that the system and surroundings can be put back in their original states by exactly reversing the process. Changes are infinitesimally small in a reversible process.
  • 26. Irreversible Processes • Irreversible processes cannot be undone by exactly reversing the change to the system. • All Spontaneous processes are irreversible. • All Real processes are irreversible.
  • 27. Energy, Work and Heat Energy is the capacity to do work. Energy classification into: kinetic potential (by motion) (by position) Is purely arbitrary! e.g.thermal chemical, electrical • Heat and work are NOT “types” of ENERGY, but are processes involving TRANSFER of energy. • They appear and disappear at the system boundary. They are path variables. • Heat is the transfer of energy from one body to another based on temperature difference. They are path variables. • Heat stimulates random motion. • Convention: if heat flows into the system, q > 0. • Work is the transfer of energy by some mechanism other than temperature difference. • They appear and disappear at the system boundary. They are path variables. • Convention: if work is done on the system, w > 0. • Work stimulates organized motion. • Work “degrades” into heat. Qualitative observations by Count Rumford (Ben Thompson) Quantitative measurements by James Joule
  • 28. Energy Concept of Internal Energy • E = K + V + U where, K and V are the macroscopic (not molecular) kinetic and potential energies of the system • U is the internal energy of the body (due to molecular motions and intermolecular interactions) • Internal Energy,U, is the total kinetic energy due to motion of molecules (translational, rotational, vibrational) the total potential energy associated with the vibrational and electric energy of atoms within molecules or crystals. • Um (molar internal energy) = U/n, where n= no. of moles of the substance • Um = Utr, m + Urot, m + Uvib, m + Uinternal, m + Urest, m (where, Urest,m = rest mass energy of electrons & nuclei = mrelC2= constant)
  • 29. Energy Properties of Internal Energy • U is a State function, a property that: Depends only on the current state of the system and is independent of how or through path that state has been reached. • It is an exact differential and its fundamental variables are V and T ⎛ ∂U ⎞ ⎛ ∂U ⎞ U = f (V, T); dU = ⎜ ∂V ⎟ dV +⎜ ∂T ⎟ dT ⎝ ⎠T ⎝ ⎠V • For cyclic process, ∫ dU =0 • U is an Extensive property
  • 30. The First Law of Thermodynamics: Work, Heat & Energy T1 → T2 T1 → T2 h Joule Experiment Joule Equivalent of Heat: 1 cal = 4.184 J
  • 31. Work • Expansion work, work of expansion (or compression) • Non-expansion / additional work: any other work where • pex = external pressure • A = piston area • dz = displacement • dV = Adz = volume change for the gas vf Total work done, w = − ∫ p ex dV vi • Work done on the system + ve i.e., Compression • Work done by the system - ve i.e., Expansion
  • 32. 1st Law of Thermodynamics Consider an example system of a piston and cylinder with an enclosed dilute gas characterized by P,V,T & n. What happens to the gas if the piston is moved inwards? Compression •If the container is insulated the temperature will rise, the atoms move faster and the pressure rises. •Is there more internal energy in the gas? Yes ∆x External agent did work in pushing the piston inward. w = - F d = -(PA) (-Δx) w = P Δ V Work done on the gas equals the change in the internal energy of the gas w = Δ U
  • 33. 1st Law of Thermodynamics • Change the situation: • Keep the piston fixed at its original location. • Place the cylinder on a hot plate. What happens to gas? • Heat flows into the gas. • Atoms move faster, internal energy increases. • Q = heat (in Joules) flows in ∆U = change in internal energy in Joules. Q = ∆U
  • 34. 1st Law of Thermodynamics F What if we added heat and pushed the piston in at the same time? • Work is done on the gas, • Heat is added to the gas and • the internal energy of the gas increases: ΔU = w + Q U INCREASES with INCREASE in TEMP. of the system, when: 1. work is done on the system by the surrounding or, 2. heat flows into the system from the surrounding or, 3. both, heat and work flows from the surr. into the system
  • 35. The First Law: Sign convention • Work done on the system by surr + ve i.e., Compression • Work done by the system by surr - ve i.e., Expansion
  • 36. Partial Differentiation: A primer Consider a function of two variables f (x,y) Definition: A partial derivative of one of the variables: the rate of change of the function w.r.t. that variable with all other variables kept fixed. Suppose: f = f (x,y), ⎛ df ⎞ f ( x + Δx,y ) − f ( x,y ) ⎜ dx ⎟ = LimΔx →0 ⎝ ⎠y Δx ⎛ df ⎞ f ( x ,y + Δy ) − f ( x,y ) ⎜ ⎟ = LimΔy →0 ⎝ dy ⎠x Δy • For example: f (x, y) = x2y ⎛ ∂f ⎞ ⎛ ∂f ⎞ ⎜∂ ⎟ = 2xy, ⎜ ⎟ = x 2 ⎝ x ⎠y ⎝ ∂y ⎠x
  • 37. Properties of partial derivatives Consider a function of two variables f (x, y) ∴ Its differential form will be: ⎛ df ⎞ ⎛ df ⎞ df = ⎜ ⎟ dx + ⎜ dy ⎟ dy ⎝ dx ⎠ y ⎝ ⎠x •The Chain rule: Let s be an independent parameter and if change of s results in changes in the values of x and y. i.e., x = x (s); y = y (s); ∴ we can write, f (x, y) ≡ f (s) df ⎛ df ⎞ dx ⎛ df ⎞ dy = ⎜ ⎟ + ⎜ ⎟ ds ⎝ dx ⎠ y ds ⎝ dy ⎠ x ds
  • 38. Properties of partial derivatives • The Cyclic Rule: If z is a function two variable, then we can write: z = z (x, y), ⎛ dy ⎞ ⎛ dz ⎞ ⎛ dx ⎞ then, ⎜ ⎜ ⎟ = −1 ⎝ dz ⎟ x ⎜ dx ⎟ y ⎠ ⎝ ⎠ ⎝ dy ⎠ z Example: If V = f (p, T); p = f (V, T); T= f (p, V), then we can write ⎛ dp ⎞ ⎛ dT ⎞ ⎛ dV ⎞ ⎜ ⎟ ⎜ ⎟ ⎜ ⎟ = −1 ⎝ dT ⎠V ⎝ dV ⎠ p ⎝ dp ⎠T Example 1: ⎛ dp ⎞ nR ⎛ dT ⎞ p ⎛ dV ⎞ nRT ⎜ dT ⎟ = ;⎜ ⎟ = ;⎜ ⎟ =− 2 ⎝ ⎠V V ⎝ dV ⎠ p nR ⎝ dp ⎠T p Use the Equation of state for Ideal gas to verify the cyclic ⎛ dp ⎞ ⎛ dT ⎞ ⎛ dV ⎞ ⎛ nR ⎞ ⎛ p ⎞ ⎛ nRT ⎞ ∴⎜ ⎟ ⎜ ⎟ ⎜ ⎟ =⎜ ⎟⎜ ⎟ ⎜− 2 ⎟ rule ⎝ dT ⎠V ⎝ dV ⎠ p ⎝ dp ⎠T ⎝ V ⎠ ⎝ nR ⎠ ⎝ p ⎠ p = nRT/V; V= nRT/p; T= pV/nR ⎛ nRT ⎞ = −⎜ ⎟ = −1 ⎝ pV ⎠
  • 39. Properties of partial derivatives •Two partial derivatives operating on a function: Let f be function of two variables, i.e., f = f (x, y); Double partial derivative of the function f can be written as: ∂ ⎛ df ⎞ ∂ 2f ∂2f ∂2f ⎜ ⎟ = = ∂x ⎝ dy ⎠ x ∂ x ∂y ∂x ∂ y ∂ y ∂x Verification: Let the function be: f ( x , y ) = x 2 y , ∴ ∂ f 2 ∂ 2f The exact differential = 2x, = 2x, ∂y ∂x ∂y ∂x •In general, the total differential form of f(x,y) may be written as: df = M( x , y )dx + N ( x , y )dy where , M = ⎛ ∂f ⎞ and ⎛ ∂f ⎞ N = ⎜ ⎜ ⎟ ⎟ ⎝ ∂x ⎠ y ⎝ ∂y ⎠ x
  • 40. Properties of partial derivatives • Does any differential form of type [M(x,y)dx + N(x,y)dy] always represent the total differential form of a function? Only if ⎛ ∂M ⎞ ⎛ ∂N ⎞ ⎜ ⎟ = ⎜ ⎟ ⎝ ∂y ⎠ x ⎝ ∂x ⎠ y Then, df = [M(x,y)dx + N(x,y)dy] represents an exact differential. Example: Let us consider: 3 x 2 y 2 dx + 2 x 3 ydy where, M( x , y ) = 3 x 2 y 2 , N ( x ,y ) = 2 x 3y It can be easily verified that the above expression corresponds to an exact differential function of the type: 3 x 2 y 2 dx + 2 x 3 ydy = d ( x 3 y 2 )
  • 41. Properties of partial derivatives Consequence: Let us move from a point (xi,yi) to another point (xf,yf) The corresponding change in f(x,y) can be written as: f f Δf = f ( xf , yf ) − f ( xi , yi ) = ∫ df i = ∫ ( Mdx i + Ndy ) • The VALUE OF THE INTEGRAL OF AN EXACT DIFFERENTIAL is INDEPENDENT OF THE PATH taken in going from initial to final point and DEPENDS only on the values of f(x, y) at the initial and the final points. NOTE: Integral of an exact differential function,df, for a closed path (i.e., cyclic) where, i (initial state) = f (final state): ∫ df = 0
  • 42. Test for Exactness (State Variable) If z = f( x,y), dz will be a perfect differential when it is found ∂z ⎞ ⎛∂z ⎞ then , dz = ⎛ ⎜ ⎟ dx + ⎜ ⎟ dy ⎝ ∂ x ⎠y ⎝ ∂ y ⎠x • dz is a single-valued function ∂z ⎛ ∂z ⎞ depending entirely on the if, ⎛ ⎞ = M ; and ⎜ ⎟ = N ⎜ ⎟ instantaneous values of x and y. ⎝ ∂x ⎠y ⎝ ∂y ⎠x then, dz = M( x,y)dx + N( x,y)dy • dz between any two specified points or states is independent of the path of transition. Then for exact differential, ⎛ ∂ M⎞ ⎛ ∂N ⎞ • dz for a complete cyclic process ⇒⎜ ⎟ = ⎜ ⎟ is equal to zero ⎝ ∂ y ⎠x ⎝ ∂ x ⎠y ⎡ ∂ ⎛∂z ⎞ ⎤ ⎡ ∂ ⎛∂z ⎞ ⎤ • δq and δw are NOT EXACT i.e., ⎢ ⎜ ⎟ ⎥ = ⎢ ⎜ ⎟ ⎥ differential quantities therefore ⎣∂ y ⎝ ∂ x ⎠y ⎦x ⎢∂ x ⎝ ∂ y ⎠x ⎦y ⎣ ⎥ they are NOT STATE Variables.
  • 43. Properties of partial derivatives
  • 44. The gas laws isotherm, curves in a graph corresponding to a single temperature. isobar, curves in a graph corresponding to a single pressure. isochore, curves in a graph corresponding to a single volume. gas constant, R (with R = NAk, where NA is Avogadro’s constant and k is Boltzmann’s constant).
  • 45. The gas law perfect/ideal gas equation, pV = nRT. perfect/ideal gas, a gas that obeys pV = nRT exactly under all conditions. real gas, an actual gas. e.g., standard ambient temperature and pressure (SATP), 298.15 K (25 °C) and 1 bar (or, 0.986 atm or 100 kPa). standard temperature and pressure (STP) 273.15 K (0 °C) and 1 bar (100 kPa, 0.986 atm.) Normal temperature and pressure (NTP) 273.15 K (0 °C) and 1 atm (101.325 kPa, 760 Torr) 1 atm =(101.325 kN/m2, 101.325 kPa, 14.7 psi, 29.92 in Hg, 760 torr).
  • 46. Partial pressure , of a gas is the pressure the gas would exert if it occupied the container alone; in general, pi = xi P Vapour pressure, the pressure of a vapour in equilibrium with its condensed phase Mole fraction, the amount of i species, expressed as a fraction of moles of the moles of ith species (ni) to the total amount of moles, n, in the sample, xi = ni/n
  • 47. partial pressure: of an ideal gas, the pressure a gas would exert if it occupied the container alone; in general, pi = xi p. Dalton’s law: The pressure exerted by a mixture of gases is the sum of the partial pressures of the gases.
  • 48. Thermodynamics Thermodynamics: → Describes macroscopic properties of equilibrium systems → Entirely Empirical → Built on 4 Laws and “simple” mathematics 0th Law Defines Temperature (T) 1st Law Defines Energy (U) 2nd Law Defines Entropy (S) 3rd Law Gives Numerical Value to Entropy These laws are UNIVERSALLY VALID, they cannot be circumvented
  • 49. Work • Expansion work, work of expansion (or compression) • Non-expansion / additional work: any other work where • pex = external pressure • A = piston area • dz = displacement • dV = Adz = volume change for the gas vf Total work done, w = − ∫ p ex dV vi • Work done on the system + ve i.e., Compression • Work done by the system - ve i.e., Expansion
  • 50. 1st Law of Thermodynamics F Consider an example system of a piston and cylinder with an enclosed dilute gas characterized by P,V,T & n. What if we added heat and pushed the piston in at the same time? • Work is done on the gas, • Heat is added to the gas and • the internal energy of the gas increases: ΔU = w + Q Statement: Change of internal energy in a closed system of is equal to the energy flow across its boundary as heat or work U INCREASES with INCREASE in TEMP. of the system, when: 1. work is done on the system by the surrounding or, 2. heat flows into the system from the surrounding or, 3. both, heat and work flows from the surr. into the system
  • 51. The First Law: Sign convention • Work done on the system by surr + ve i.e., Compression • Work done by the system by surr - ve i.e., Expansion Alternate Statement: If a system is subjected to a CYCLIC Transformation, the work produced in the surroundings is equal to the heat withdrawn from the surroundings. Q = -w (change in U is zero as it’s a State function) If w is +ve (compression, work done on the system) then q will be –ve (heat will be released by the system) and vice versa
  • 52. Work • Expansive work, work of expansion (or compression) • Non-expansive / additional work : any other work piston held down by F= mg pins pex= mg/A F= pex.A m dz Area =A Pi , Vi Pf , Vf w = - mg.A.dz w = - mg.dV w = - pex.dV =-pex (Vf-Vi)
  • 53. WORK Reversible Isothermal Expansion : w = − ∫ ( pex − dp)dV = − ∫ ( pdV − dpdV ) = − ∫ pdV dV Vf where, p = p(V) w = −nRT ∫ = −nRT ln p = nRT/V V Vi Irreversible Isothermal Expansion: Vf w = − pex ∫ dV = − pex (V f − Vi ) = − pex ΔV Vi
  • 55.
  • 56.
  • 57. Irreversible Reversible Expansion Irreversible Reversible Compression • For a reversible process Work on expansion = work of compression (same path) • For an irreversible process Work on expansion ≠ work of compression (same path)
  • 58. Work wrev > wirr • Work done on expansion by the system on surroundings (sign negative) operating between specified initial and final states and passing through and specified path is maximum work available from a system when the changes take place reversibly • For a reversible process Work on expansion = work of compression (same path) • For an irreversible process Work on expansion ≠ work of compression (same path) • Work is a path dependent parameter, path function(so as Heat)
  • 59. State and Path Functions • Some state functions, e.g., U and H etc. – Value of a state function is independent of Path 2 - Non- path adiabatic w≠0;q≠0 – Depends only on initial and final state, Path 1 - e.g. ΔU = Ufinal - Uinitial Adiabatic w≠0;q=0 – Overall Change final ΔU = ∫ dU ⇒ dU is an exact differential initial • Path from initial to final state has a functional dependence – For ∆U, work may be done, or, heat may flow or, both – Equations that describe how you get to final ΔUpath1 = ΔUpath2 = Uf -Ui state are path functions – Path functions are path specific ∂q ⇒ ∂q is final q=∫ an inexact differential initial,path
  • 60. Work is a STATE FUNCTION? Assume a Reversible process so that pext = p where, Ar (gas) under goes change of state through compression, from Ar (g, p1, V1) (initial) → Ar (g, P2, V2) (final); such that V1 > V2 and p1< p2 Compression through two paths 1st Path: Ar(g, p1, V1) → Ar(g, p1, V2) → Ar(g, p2, V2) First V1 → V2 when p held constant at p1; then p1 → p2 when V held constant at V2 2nd Path: Ar(g, p1, V1) → Ar(g, p2, V1) → Ar(g, p2, V2) First p1 → p2 when V held constant at V1; then V1 → V2 when p held constant at p2 Note for the closed cycle, total work = w[path (1)] - [path (2)]
  • 61. Work is a STATE FUNCTION? V2 V2 w( 1) = − ∫ pextdV − ∫ pextdV V1 V2 V2 w( 1) = − ∫ p1dV = − p1(V − V ) = p1(V − V ) 2 1 1 2 V1 V1 V2 w( 2 ) = − ∫ pextdV − ∫ pextdV V1 V1 V2 w( 2 ) = − ∫ p2dV = − p2 (V − V ) = p2 (V − V ) 2 1 1 2 V1 NOTE: • Work done on the system to compress it is NOT EQUAL through the two paths. i.e., w(1) ≠ w (2) • ∴ Net work done on the system in the complete cycle ≠ 0 i.e., [w(1) - w(2)] ≠ 0; ∫ ∂w ≠ 0 (closed cycle) • This means w is NOT a state function ∴ we CAN NOT write w = f(V, p)
  • 62. Ideal gas, closed system, reversible process Calculate wf and wb isothermal 10 Pa, 1 m3 , T 1 Pa, 10 m3, T isochoric 10 Pa, 1 m3, T 1 Pa, 1 m3, T2 1 Pa, 10 m3, T isobaric isobaric 10 Pa, 1 m3, T 10 Pa, 10 m3, T3 1 Pa, 10 m3, T isochoric
  • 63. 25 L of gas is enclosed in a cylinder/piston apparatus at 2 atm of pressure and 300 K. A 100 kg of mass is placed on the piston causing the gas to compress to 20 L at constant pressure. This is done by allowing heat to flow out of the gas. What is the work done on the gas? What is the change in internal energy of the gas? How much heat flowed out of the gas? • Po = 202,600 Pa, Vo = 0.025 m3, • To = 300 K, Pf = 202,600 Pa, • Vf=0.020 m3, Tf= ? • n = PV/RT W = -P∆V ∆ U = 3/2 nR ∆T Q = W + ∆ U W = - P ∆ V = -202,600 Pa (0.020 – 0.025)m3 = 1013 J energy added to the gas ∆ U =3/2 nR ∆T=1.5(2.03)(8.31)(-60)= -1518 J Q = W + ∆ U = 1013 – 1518 = -505 J heat out
  • 64. Heat Transactions In general change in the internal dU = dq + dw exp + dw add energy of a closed system is given by - For dV = 0; dwexp = 0 and if dwadd = 0, then dU = dq (constant volume, no additional work) = dqv For a measurable change, ΔU = qv -heat capacity, C, the ratio of heat supplied to the temperature rise it causes. C = dq/dT; C = q/ ΔT - heat capacity at constant volume, CV = (∂U/∂T)V - molar heat capacity, the heat capacity divided by the amount of substance, Cm = C /n. adiabatic bomb calorimeter - specific heat capacity, the heat capacity divided by the mass, Cs = C /m
  • 65. Heat Capacity for Constant Volume Processes (Cv) insulation ΔT Heat, Q m added m • Heat is added to a substance of mass m in a fixed volume enclosure, which causes a change in internal energy, U. Thus, Q = U2 - U1 = ∆U = m Cv ∆T The v subscript implies constant volume
  • 66. Heat Capacity for Constant Pressure Processes (Cp) Δx ΔT Heat, Q m added m • Heat is added to a substance of mass m held at a fixed pressure, which causes a change in internal energy, U, AND some PV work.
  • 67. Heat Transactions and Enthalpy For dV ≠ 0; dwexp≠ 0 even if dwadd = 0, then dU ≠ dq ΔU = qp - pΔV qp = ΔU +pΔV = U2 – U1 + p(V2 – V1) = (U2 + pV2) – (U1 + pV1) Define H = U + pV •Differential scanning calorimeter dH = dU + pdV + Vdp •Isobaric calorimeter = dU - w (at constant p) •Adiabatic flame calorimeter = dqp At constant p, dH = dqp (constant pressure, no additional work) - Heat capacity at constant pressure, Cp = (∂H/∂T)p - Enthalpy change and temperature change, dH = nCp,m dT; ΔH = nCp,m ΔT (if Cp independent of T) Empirical expression, Cp,m = a + bT + c/T2
  • 68. Heat Transactions - for ideal/perfect gas; relation between ∆U and ∆H, ∆H = ∆U + ∆ngRT. - relation between heat capacities of a perfect gas, Cp – CV = nR
  • 69. For any process U = f (V , T ) H = f ( P, T ) ⎛ ∂U ⎞ dU = ⎜ ⎛ ∂U ⎞ ⎟ dV + ⎜ ⎛ ∂H ⎞ ⎛ ∂H ⎞ ⎟ dT dH = ⎜ ⎟ dP + ⎜ ⎟ dT ⎝ ∂V ⎠T ⎝ ∂T ⎠V ⎝ ∂P ⎠ T ⎝ ∂T ⎠ P = π T dV + CV dT ⎛ ∂H ⎞ =⎜ ⎟ dP + C P dT ⎛ ∂U ⎞ ⎝ ∂P ⎠T πT = ⎜ ⎟ Internal pressure ⎝ ∂V ⎠ T dU = CV dT (for ideal gas) dH = Cp dT (for ideal gas) For ideal gas ⎛ ∂U ⎞ For ideal gas πT = ⎜ ⎟ =0 ⎛ ∂H ⎞ ⎝ ∂V ⎠T ⎜ ⎟ =0 ⎝ ∂P ⎠T Joule Experiment
  • 70. Adiabatic Reversible Process for ideal gas, Cv independent of Temp 1 dU = dw + dq = dw CV nR ⎛ T2 ⎞ ⎛ V1 ⎞ T2 ⎛ V1 ⎞ C ⎜ ⎟ =⎜ ⎟ c ⎜T ⎟ ⎜V ⎟ = ⎜ ⎟ where c = V ,m Cv dT = − pdV ⎝ 1⎠ ⎝ 2⎠ T1 ⎜ V2 ⎟ ⎝ ⎠ R CV nR C p −CV T2 dT V2 dV ⎛ T2 ⎞ ⎛V ⎞ ⎛V ⎞ Cv ∫ = - nR ∫ ⎜ ⎟ ⎜T ⎟ =⎜ 1 ⎟ ⎜V ⎟ =⎜ 1 ⎟ ⎜V ⎟ T1 T V1 V ⎝ 1⎠ ⎝ 2⎠ ⎝ 2⎠ γ −1 T2 V1 T2 ⎛ V1 ⎞ C p ,m Cv ln = nR ln =⎜ ⎟ where γ = T1 V2 T1 ⎜ V2 ⎟ ⎝ ⎠ CV ,m TV γ −1 = constant PV γ = constant VT c = constant T γ P 1−γ = constant
  • 71. Conclusion of Ist Law of Thermodynamics • The internal energy of an isolated system is a constant For isolated system : dU = 0; (as q = 0, w = 0» No perpetual motion machines! ) • The energy of the universe is constant. ∆Usystem = −∆Usurroundings • When a system undergoes a process that leads to a change of state then the sum of the heat q transferred and the work w performed, is equal to the change in the internal energy dU of the system. dU = ∂q + ∂w (Closed system, through a number of steps) • A system contains ONLY internal energy. A system does not contain heat or work.
  • 72. Conclusion of Ist Law of Thermodynamics • Cyclic Process ∫ dU =0 (Exact differential) • In a cyclic process the work done by a system on its surroundings is equal to the heat withdrawn from the surroundings . - δ w = δq • For an Adiabatic Process δ wad = dU ; (as δq = 0) • For a Non-Adiabatic Process δq = dU − δw ≡ δq = (δwad – δw); (as, δwad = dU)
  • 73. Calculation of thermodynamic functions for various processes reversible phase const p heating, no const V heating, no change at const. T, p phase change phase change w − ∫ p dV = − pΔV − ∫ p dV = − pΔV 0 q latent heat q p = ΔH qV = ΔU ΔU q + w q + w = ∫ CV (T )dT ΔH q = ∫ C p (T )dT ΔU + VΔp
  • 74. Calculation of thermodynamic function for various processes for Ideal Gas Reversible, no phase change rev, isothermal rev, adiabatic rev rev, const irrev, const ext. p final p w − nRT ln V2 = ∫ CV (T )dT − ∫ PdV − pex ΔV − p f ΔV V1 q ΔU-w nRT ln V2 0 V1 ΔU = ∫ CV (T )dT 0 = ∫ CV (T )dT ΔH = ∫ C p (T )dT 0 = ∫ C p (T )dT
  • 75.
  • 76.
  • 77.
  • 78.
  • 79. SUMMRAY OF ADIABATIC WORK (with solved example) • Reversible Adiabatic Expansion (or compression) of an Ideal Gas 1 mole gas (V1,T1) = 1 mole gas (V2,T2) adiabatic ⇒ đq = 0 Reversible ⇒ đw = -pd V Ideal gas ⇒ dU = Cv d T ∴ From 1st Law dU = -pd V ⇒ CvdT = -pdV along path dT dV CV dT = − pdV ⇒ CV = −R p =RT T V V Cp R CV −1 T2 dT V dV ⎛T2 ⎞ ⎛V1 ⎞ C p −CV =R for i.g. ⎛T2 ⎞ ⎛V1 ⎞CV CV ∫ = −R ∫ 2 ⇒ ⎜ ⎟=⎜ ⎟ ⎯⎯⎯⎯⎯⎯→ ⎜ ⎟=⎜ ⎟ T1 T V V 1 ⎝T1 ⎠ ⎝V2 ⎠ ⎝T1 ⎠ ⎝V2 ⎠ γ −1 Cp ⎛T2 ⎞ ⎛V1 ⎞ Define γ ≡ ⇒ ⎜ ⎟ = ⎜ ⎟ CV ⎝T1 ⎠ ⎝V2 ⎠ 3 ⎫ CV = R ⎪ 2 ⎪ 5 For monatomic ideal gas: ⎬ γ = ( > 1 generally) 5 ⎪ 3 Cp = R 2 ⎪⎭ In an adiabatic expansion (V2 > V1), the gas cools (T2 > T1). And in an adiabatic compression (V2 < V1), the gas heats up. γ pV ⎛ p2 ⎞ ⎛V1 ⎞ For an ideal gas (one mole) T = ⇒ ⎜ ⎟=⎜ ⎟ ⇒ pV1 γ = pV2γ R ⎝ p1 ⎠ ⎝V2 ⎠ 1 2 pV γ is constant along a reversible adiabat For an isothermal process T = constant ⇒ pV = constant
  • 80. p p1 V2adiabat < V2isotherm because the gas cools during reversible p2 adiabatic expansion V1 V2ad V2iso • Irreversible Adiabatic Expansion of an ideal gas against a constant external pressure 1 mol gas (p1,T1) = 1 mol gas (p2,T2) (pext=p2) adiabatic ⇒ đq = 0 Constant pext = p2 ⇒ đw = -p2dV Ideal gas ⇒ dU = CvdT 1st Law ⇒ dU = -p2dV ∴ Cv d T = - p2 dV Integrating: Cv ( T2 - T 1 ) = - p2 ( V2 - V1 ) ⎛ p2 ⎞ Using pV = RT T2 (CV + R ) =T1 ⎜ CV + R⎟ ⎝ p1 ⎠ Note p2 < p1 ⇒ T2 < T1 Again, expansion cools Note also (-wrev) > (-wirrev) Less work is recovered through an irreversible process
  • 81. Some Thermodynamic Cycles đq • Reversible Ideal Gas processes: Find ∆U , ∆H , q , w , ∫T (I ) (II) p p (T ) 1 (T ) 1 D (const. p) (T ) 3 p1 p1 A (isotherm) B (T ) A E (const. V) p2 1 p2 p3 (rev. C (const. V) (isotherm) (T ) 1 adiabat) (T ) 2 V1 V2 V1 V2 const. T [A] 1 mol gas (p1,V1,T1) = 1 mol gas (p2,V2,T1) Ideal gas isotherm: ∆UA = 0 ∆HA = 0 as, ΔH = Cp ΔT = 0 V V đ qA V2 wA = −RT1 ln 2 qA = RT1 ln 2 ∫T = R ln V1 V1 V1 rev.adiabat [B] 1 mol gas (p1,V1,T1) = 1 mol gas (p3,V 2,T2) Adiabat: qB = 0 ∆UB = CV (T2 −T1 ) Ideal gas: ∆HB = C p (T2 −T1 ) 1st Law: w B = CV (T2 −T1 ) đqB ∫T =0
  • 82. reversible [C] 1 mol gas (p3,V2,T2) = 1 mol gas (p2,V2,T1) const. V ∆UC = CV (T1 −T2 ) Constant V: wC = 0 Ideal gas: ∆HC = C p (T1 −T2 ) 1st Law: qC = CV (T1 −T2 ) đqC ⎛T ⎞ ∫T = CV ln ⎜ 1 ⎟ ⎝T2 ⎠ [A] vs. [B] + [C] ∆UA = 0 ∆UB + ∆UC = 0 = ∆UA ∆HA = 0 ∆HB + ∆HC = 0 = ∆HA V qA = RT1 ln 2 qB + qC = CV (T1 −T2 ) ≠ qA V1 V w A = −RT1 ln 2 wB + w C = CV (T2 −T1 ) ≠ w A V1 đqA V2 đqB đqC ⎛V ⎞ đq ∫T = R ln ∫T +∫ = R ln ⎜ 2 ⎟ = ∫ A V1 T ⎝V1 ⎠ T ⎛ đq ⎞ This result suggests that ⎜ ∫ rev ⎟ is a state function! ⎝ T ⎠ ∆UD = CV (T3 −T1 ) [D] qD = C p (T 3 − 1 T ) ∆H D = C p(T 3−T 1) đqD ⎛T ⎞ wD = −R (T3 −T1 ) ∫T = C p ln ⎜ 3 ⎟ ⎝T1 ⎠
  • 83. ∆UE = CV (T1 −T3 ) [E] wE = 0 qE = CV (T1 −T3 ) ∆HE = C p (T1 −T3 ) đqE ⎛T ⎞ ∫T = CV ln ⎜ 1 ⎟ ⎝T3 ⎠ [A] vs. [D] + [E] ∆UA = 0 ∆UD + ∆UE = ∆UA ∆HA = 0 ∆HD + ∆HE = ∆HA V qA = RT1 ln 2 qD + qE = R (T3 −T1 ) ≠ qA V1 V w A = −RT1 ln 2 wD + w E = −R (T3 −T1 ) ≠ w A V1 đqA V2 đqD đqE ⎛V ⎞ đq ∫T = R ln ∫T +∫ = R ln ⎜ 2 ⎟ = ∫ A V1 T ⎝V1 ⎠ T ⎛ đq ⎞ Here again ⎜ ∫ rev ⎟ looks like a state function! ⎝ T ⎠
  • 84. Conclusion of Ist Law of Thermodynamics • The internal energy of an isolated system is a constant For isolated system : dU = 0; (as q = 0, w = 0» No perpetual motion machines! ) • The energy of the universe is constant. ∆Usystem = −∆Usurroundings • When a system undergoes a process that leads to a change of state then the sum of the heat q transferred and the work w performed, is equal to the change in the internal energy dU of the system. dU = ∂q + ∂w (Closed system, through a number of steps) • A system contains ONLY internal energy. A system does not contain heat or work.
  • 85. Conclusion of Ist Law of Thermodynamics • Cyclic Process ∫ dU =0 (Exact differential) • In a cyclic process the work done by a system on its surroundings is equal to the heat withdrawn from the surroundings . - δ w = δq • For an Adiabatic Process δ wad = dU ; (as δq = 0) • For a Non-Adiabatic Process δq = dU − δw ≡ δq = (δwad – δw); (as, δwad = dU)
  • 86.
  • 87. Calculation of thermodynamic functions for various processes reversible phase const p heating, no const V heating, no change at const. T, p phase change phase change w − ∫ p dV = − pΔV − ∫ p dV = − pΔV 0 q latent heat q p = ΔH qV = ΔU ΔU q + w q + w = ∫ CV (T )dT ΔH q = ∫ C p (T )dT ΔU + VΔp
  • 88. Calculation of thermodynamic function for various processes for Ideal Gas Reversible, no phase change rev, isothermal rev, adiabatic rev rev, const irrev, const ext. p final p w − nRT ln V2 = ∫ CV (T )dT − ∫ PdV − pex ΔV − p f ΔV V1 q ΔU-w nRT ln V2 0 V1 ΔU = ∫ CV (T )dT 0 = ∫ CV (T )dT ΔH = ∫ C p (T )dT 0 = ∫ C p (T )dT
  • 89. Variation of U with system variables: U = f (V , T ) ⎛ ∂U ⎞ dU = ⎜ ⎛ ∂U ⎞ ⎟ dV + ⎜ ⎟ dT ⎝ ∂V ⎠T ⎝ ∂ T ⎠V 1. Change in U w.r.t. T at constant volume ⎛ ∂U ⎞ Cv = ⎜ ⎟ ; qv = Cv ΔT = ΔU ⎝ ∂T ⎠ V ⎛ ∂U ⎞ 2. Change in U w.r.t. V at constant temp: ⎜ ⎟ ⎝ ∂V ⎠ T = π T dV + C V dT For real gas dU = CV dT (for ideal gas) As For ideal gas π T = ⎜ ⎛ ∂U ⎞ ⎟ =0 ⎝ ∂V ⎠T 3. Change in U w.r.t. T at constant pressure ⎛ ∂U ⎞ dU = Cv dT + ⎜ ⎟ dV ⎛ ∂U ⎞ ⎛ ∂U ⎞ ⎝ ∂V ⎠ T ⎜ ⎟ = Cv + αV ⎜ ⎟ ⎝ ∂T ⎠ P ⎝ ∂V ⎠ T ⎛ ∂U ⎞ ⎛ ∂U ⎞ ⎛ ∂ V ⎞ ⎜ ⎟ = Cv + ⎜ ⎟ ⎜ ⎟ ⎝ ∂T ⎠ P ⎝ ∂V ⎠ T ⎝ ∂T ⎠ P where
  • 90. Change in Internal Energy at Constant P • Suppose we want to know how the internal energy, U, changes with temperature at constant pressure dU = π dV + C dT T V ⎛ ∂U ⎞ ⎛ ∂ (π T dV + C V dT)⎞ ⎜ ⎟ =⎜ ⎟ ⎝ ∂T ⎠ p ⎝ ∂T ⎠p ⎛ ∂U ⎞ ⎛ ∂V ⎞ ⎜ ⎟ = π T ⎜ ⎟ + CV ⎝ ∂T ⎠ p ⎝ ∂T ⎠ p – But the change in volume with temperature at constant pressure is related to the Isobaric thermal expansion / expansion coefficient of the gas, α 1 ⎛ ∂V ⎞ ⎛ ∂V ⎞ α= ⎜ ⎟ or ⎜ ⎟ = αV V ⎝ ∂T ⎠ p ⎝ ∂T ⎠ p ⎛ ∂U ⎞ so ⎜ ⎟ = π Tα V + C V ⎝ ∂T ⎠ p • Large α means sample responds strongly to changes in T • For an ideal gas, πT = 0 so ⎛ ∂U ⎞ ⎜ ⎟ = CV [definition ] ⎝ ∂T ⎠ p
  • 91. Variation of V with system variables: Experimentally known that the Volume of an isotropic material is a function of Temperature and Pressure. isothermal compressibility relative/fractional coefficient of Isobaric change of Volume thermal expansion / expansion coefficient For an ideal gas : PV = nRT similarly κT = 1/p For solid and liquid α and κT are approx. independent of T & p
  • 92. Another quantity of interest which can be obtained from α and κT is: This derivative tells us how fast the pressure rises when we try to keep the volume constant while increasing the temp. Exercise: How much pressure would be generated in a mercury thermometer if we tried to heat the thermometer higher than the temperature where the mercury has reached the top of the thermometer. Given: For Hg, α = 1.82 Ø 10×4 K×1 and κT = 3.87 Ø 10×5 atm×1 We see that each 1 C increases the pressure by 4.7 atm, about 69 lb/sq in. This is a lot of pressure for a glass tube to withstand. It wouldn't take very many degrees of temperature increase to break the glass thermometer.!!! Using a variation of Euler's chain rule we can write
  • 93. Variation of H with system variables: H = f ( P, T ) dH = ⎛ ∂H ⎞ dP+⎛ ∂H ⎞ dT ⎜ ⎟ ⎜ ⎟ ⎝ ∂P ⎠T ⎝ ∂T ⎠ P 1. Change in H w.r.t. T at constant pressure ⎛ ∂H ⎞ C p = ⎜ ⎟ ; q p = C p ΔT = ΔH ⎝ ∂T ⎠ P ⎛ ∂H ⎞ 2. Change in H w.r.t. P at constant temperature: ⎜ ⎟⎝ ∂P ⎠ T H = f ( P, T ) ⎛ ∂H ⎞ Alternately, = ⎜ ⎟ dP + CP dT ⎛ ∂H ⎞ ⎛ ∂P ⎞ ⎛ ∂T ⎞ ⎝ ∂P ⎠T ⎜ ⎟ ⎜ ⎟ ⎜ ⎟ = −1 ⎝ ∂P ⎠ T ⎝ ∂T ⎠ H ⎝ ∂H ⎠ P dH = Cp dT (for ideal gas) ⎛ ∂H ⎞ ⎛ ∂T ⎞ ⎛ ∂H ⎞ ∴ ⎜ ⎟ = −⎜ ⎟ ⎜ ⎟ = − μ JT C p ∂H ⎞ ⎝ ∂P ⎠ T ⎝ ∂P ⎠ H ⎝ ∂T ⎠ P For ideal gas ⎛ ⎜ ⎟ = 0 ⎝ ∂P ⎠T 3. Change in H w.r.t. T at constant volume: ⎛ ∂H ⎞ ⎜ ⎟ ⎛ ∂H ⎞ ⎝ ∂T ⎠ V dH = C P dT + ⎜ ⎟ dP ⎝ ∂P ⎠ T ⎛ ∂H ⎞ ⎛ ∂P⎞ α ⎛ ∂H ⎞ ⎛ ∂H ⎞ ⎛ ∂ P ⎞ From earlier results ⎜ ⎟ = −μ JT Cp ; ⎜ ⎟ = ⎜ ⎟ = CP + ⎜ ⎟ ⎜ ⎟ ⎝ ∂P ⎠ T ⎝ ∂T ⎠ V κ ⎝ ∂T ⎠ V ⎝ ∂P ⎠ T ⎝ ∂T ⎠ V ⎛ ∂H ⎞ ⎡ αμ ⎤ ∴⎜ ⎟ = CP ⎢1 − JT ⎥ ⎝ ∂T ⎠ V ⎣ κ ⎦
  • 94. The Joule-Thomson Expansion Expt The Joule-Thomson experiment consists of forcing a gas at constant backing pressure passing through a porous plug under adiabatic condition and measuring the change in temperature. ⎛ ∂T ⎞ ≈ ΔT The Joule-Thomson coefficient (μJT ) = ⎜ ⎟ ⎝ ∂P ⎠ H Δp The most straightforward way to measure the coefficient is to measure the temperature of the gas entering and leaving the porous plug and divide the change in temperature by the change in pressure: we need to decide what is being held constant when we take the partial derivative. In this case, since q =0, the change in internal energy of the gas is equal to w.
  • 95. Joule-Thompson Experiment: Inversion Temperature In this experiment q = 0 w = - pf (Vf – 0) - pi (0 - Vi) ΔU = Uf – Ui = q + w = - pfVf + piVi Uf + pfVf = Ui + piVi Hf = Hi , ΔH = 0 Isenthalpic process ⎛ ∂H ⎞ ⎛ ∂H ⎞ H = f ( P, T ); dH = ⎜ ⎟ dP + ⎜ ⎟ dT ⎝ ∂P ⎠T ⎝ ∂T ⎠ P ⎛ ∂H ⎞ ⎛ ∂H ⎞ ⎛ ∂T ⎞ ⎜ ⎜ ∂p ⎟ ⎟ = −⎜ ⎟ ⎜ ⎟ = −C p × μ ⎜ ⎟ Applying Euler’s Chain Rule, we get: ⎝ ⎠T ⎝ ∂T ⎠ p ⎝ ∂p ⎠ H Joule-Thompson Coefficient , μ (or μJT ) = ⎛ ∂T ⎞ ≈ ΔT in this J-T expt. ⎜ ⎟ ⎝ ∂P ⎠ H Δp ⎛ ∂H ⎞ ⎛ ∂H ⎞ H = f ( P, T ); dH = ⎜ ⎟ dP + ⎜ ⎟ dT dH = − μC p dP + C p dT ⎝ ∂P ⎠T ⎝ ∂T ⎠ P
  • 96. THE JOULE-THOMPSON EXPERIMENT ⎛ ∂T ⎞ μ =⎜ ⎟ ⎜ ∂p ⎟ ⎝ ⎠H If μ > 0 then this indicates that the gas cools (-ve δT) when gas expanded (-ve δp). If μ < 0 then this indicates that the gas heats (+ve δT) when expanded (-ve δp). The "inversion temperature" indicates where on a (T, p) isenthalpic plot the (dT/dP)H flips from +ve to –ve. Or,point where µ changes sign from + to – ve and the point is the maximum inversion temperature For a real gas µ is non-zero (except at the maximum inversion temperature)
  • 97. 2 ⎛ ∂T ⎞ 2 μ=⎜ ⎜ ⎟ ⎝ ∂p ⎟ H ⎠ The Linde process
  • 98. Joule-Thompson ⎛ ∂T ⎞ ≈ ΔT Coefficient , μ (or μJT ) = ⎜ ∂P ⎟ ⎝ ⎠ H Δp • µ can be either (+) or (-) – Positive µ means dT is negative when dp is negative •Gas cools on expansion – Negative µ means that means dT is positive when dp is negative •Gas warms on expansion – Transition between positive and negative µ is called the Joule- Thompson inversion temperature •Gases have both high and low inversion temperatures – Ideal gas µ = 0, T unchanged by Tinversion µ change in p on expansion Gas (K) (K atm-1) CO2 1500 1.11 • Practical applications: N2 621 0.25 – Gas liquefaction He 621 0.25 – Isotope separation
  • 99. ⎛ ∂T ⎞ T ( ∂V ∂ T )P −V μJT =⎜ ⎟ = ⎝ ∂ P ⎠H CP
  • 100. ⎛ ∂T ⎞ T ( ∂V ∂ T )P −V μJT =⎜ ⎟ = ⎝ ∂ P ⎠H CP
  • 101. For a van der Waal gas: Therefore, μJT depends critically on ⎛ ∂T ⎞ T ( ∂V ∂ T )P − V μJT =⎜ ⎟ = the constants a and b, which are the ⎝ ∂ P ⎠H CP indices of non zero interaction and μJT = 1 ⎛ 2a ⎞ − b⎟ finite volume of the gas molecules ⎜ CP ⎝ RT ⎠ 2a If , > b then μ > 0 (cooling observed ) RT • If initial Temp (Ti) is below 2a Tinversion only then cooling is If , < b then μ < 0 ( heating observed ) RT observed. Inversion temperature • And the final temp T2 is μ JT = 0 when T = Tinversion lower than T1 1 ⎡ 2a ⎤ ⎛ 2a ⎞ ∴ 0= ⎢ − b⎥ or , ⎜ ⎜ RT ⎟=b ⎟ Cp ⎣ RT ⎦ ⎝ inversion ⎠ 2a ∴ Tinversion = Rb
  • 102. N2 and O2 will cool upon expansion at room temperature, but He and Ne will warm upon expansion at room temperature.
  • 103. Derive the Following expressions For ideal gas ⎛ ∂P ⎞ α 1 ⎛ ∂H ⎞ ⎜ ⎟ = ∴μ JT =− ⎜ ⎟ ⎝ ∂T ⎠V κ C p ⎝ ∂P ⎠ T ⎛ ∂T ⎞ T ( ∂V ∂ T )P −V α TV 2 μJT =⎜ ⎟ = C p − CV = ⎝ ∂ P ⎠H CP κ for ideal gases : μJT = 0 1 ⎛ 2a ⎞ μJT = − b⎟ C P ⎜ RT ⎝ ⎠ ⎛ ∂H ⎞ Isothermal Joule-Thompson Coefficient, μT = ⎜ ⎟ μT = - Cpμ ⎝ ∂P ⎠T Monoatomic ideal gas CV,m = 3R/2, Cp,m = 5R/2
  • 104. The Perfect gas and πT, α, κT, μ Property PD Value for Perfect Gas Info: Internal ⎛ ∂U ⎞ Pressure πT = ⎜ ⎟ ∂V ⎠T πT=0 Strength/nature of ⎝ interactions between molecules Expansion 1 ⎛ ∂V ⎞ α =1 / T The higher T, the less Coefficient α= ⎜ ⎟ responsive is its volume V ⎝ ∂T ⎠ p to a change in temperature 1 ⎛ ∂V ⎞ Isothermal κT = − V⎝ ⎜ ⎜ ∂p ⎟ ⎟ κT=1 / p The higher the p, the Compressibility ⎠T lower its compressibility ⎛ ∂T ⎞ Joule-Thomson μ =⎜ ⎜ ⎟ ⎟ μ=0 Another indication of Coefficient ⎝ ∂p ⎠ H molecular interactions.
  • 105. Ist Law of Thermodynamics: • The different forms of energy are inter convertible. • When one form of energy disappears an equivalent of another kind must appear. Conversion of energy. • Energy can be transferred / transformed, keeping the total energy fixed. qsys = - qsurr ΔU = q + w (= – pexdV) wsys = - wsurr ∆U = q – pexdV Incompleteness of Ist Law: It Does not say anything about: • Whether any transfer / transformation of energy would occur at all? • If it does, then in which direction would the change occur? • If any transfer / transformation of energy occurs in a particular direction, then how long will it be sustained? • If any transfer / transformation of energy occurs in a particular direction, then how fast will it proceed?
  • 106. What happens when ? Free Expansion of Gas Gas Gas Valve Gas Vacuum Valve Closed Open Gas 1 Gas 2 Gases tend to occupy the whole available Ideal gas mixture ΔH=0 volume of the container. Two questions: 1) Does the enthalpy of the system increase or decrease and how much ? 2) Does the system become more or less disordered and by how much? The driving force of such a process is the increase of the disorder in the system.
  • 107. Warm Thermal Conduction The two liquids (with very similar molecules) form an ideal solution (ΔH ≈ 0), in which the molecules are randomly and uniformly mixed. Hot dQ Cold Suppose two bodies are brought in contact. Then from the Ist law, we ONLY know if q heat was lost by one, exactly q heat would be gained by the other. The law does not specify if the Ist one will lose heat or, the other one. To know the direction of flow of heat, we need another information, namely the temp of the two bodies.
  • 108. First Law of Thermodynamics • Conservation of Energy • Says Nothing About Direction of Energy Transfer Second Law of Thermodynamics • Preferred (or Natural) Direction of Energy Transfer • Determines Whether a Process Can Occur • Thermodynamic Processes can be classified into Three Types : – Natural (or Irreversible) – Impossible – Reversible
  • 109. Disorder increase for the following processes: • Solids melt to liquids • Solids or liquids vaporize to form gases • Solids or liquids dissolve in a solvent to form non-electrolyte solution • A substance is heated (increased temperature increases the molecular motions and the disorder) • A chemical reaction produces an increase in the number of molecules of gases • The 2 Law puts forward the criteria for the direction of the nd spontaneous chemical/ physical change of a thermodynamic system. • The historical roots of the second law stems from the invention of heat engine (namely, the steam engine). It is known that work can be fully converted to heat (joule’s expt), the question is can heat be converted to work???
  • 110. Entropy • The thermodynamic property of a system that is related to its degree of randomness or disorder is called entropy (S). • The entropy S and the entropy change ΔS=S2-S1 are state functions • The entropy S has a unique value, once the pressure P, the temperature T and the composition n of the system are specified, S = S (p,T,n) • The entropy is an extensive property, i.e. increases with the amount of matter in the system.
  • 111. Carnot Engine: Introduction to Heat Engines • One of the primary applications of thermodynamics is to Turn heat into work • The standard heat engine works on a reversible cyclic process: 1. extract heat from a hot reservoir, 2. perform work, 3. dump excess heat into a cold reservoir (often the environment). A “reservoir” is a large body whose temperature doesn’t change when it absorbs or gives up heat Carnot and then by Clausius: Statement of the Second law : It states that it is impossible to construct a device that operates in a cycle and produces no effect other than the transfer of heat from a lower-temperature body to a higher-temperature body.
  • 112. TH TH QH QH R WOUT HE WOUT QL QL TL TL −W Thermal efficiency = ε = QH For a complete cycle: dU = 0 ∴ Qcy = - Wcy Qcy = QH - Qc −W QH − Qc ∴ε cyc = QH = QH Q = 1− c QH The engine will have 100% efficiency only when Qc = 0
  • 113. Heat Engines • By conservation of energy: |QH| = |W| + |QL|. • The high and low temperatures TH and TL are called the operating temperatures of the engine. • We will considering only engines that run in a repeating cycle, that is, the system returns repeatedly to its starting point, and thus can run continuously. • Absolute value signs are used because we are interested only in the magnitudes.
  • 114. Second Law of Thermodynamics. The Carnot Cycle. • The Carnot cycle is an example of a reversible process, which is a process that can be done in reverse. • A reversible process requires that any changes are made infinitely slowly. • Real processes are not reversible due to friction , turbulence in the gas, etc.
  • 115. Second Law of Thermodynamics: The Carnot Cycle
  • 116. Four steps • Isothermal expansion: a to b • Adiabatic expansion: b to c • Isothermal compression: c to d • Adiabatic compression: d to a Define the efficiency ε work done by system " work" ε ≡ = heat extracted from reservoir " cost" Valid for all heat engines. W QC efficiency = ε = = 1− (∆U = 0 for closed cycle) QH QH where, W = │QH│ - │Qc│; following conservation of energy
  • 117. The Carnot Cycle • Step 1: a to b. – The gas is in contact with a heat bath at temperature TH and weight is removed from the piston. – The gas expands, while maintaining a constant Vb temperature, isothermal w1 = − nRTH ln Va – the change in the internal energy is thus equal to zero dU = 0 w1 = − q1
  • 118. The Carnot Cycle • Step 2: b to c. – The gas is isolated from the environment and some more weight is removed from the piston. – The gas expands and during the adiabatic expansion, the temperature of the gas will decrease. γ −1 γ −1 TH Vb = TLVc – For adiabatic expansion pVγ is constant, and we can w2 = nCV (TL − TH ) thus related state b to state c: q2 = 0
  • 119. The Carnot Cycle • Step 3: c to d. – The gas is in contact with a heat bath at temperature TC and weight is added to the piston. – The gas is compressed, while maintaining a constant Vd temperature, isothermal w3 = − nRTL ln Vc – the change in the internal energy is thus equal to dU = 0 zero w3 = − q3
  • 120. The Carnot Cycle • Step 4: d to a. – The gas is isolated from the environment and some more weight is added to the piston. – The gas is compressed and during the adiabatic compression, the temperature of the gas will increase. γ −1 γ −1 TH Va = TLVd w4 = nCV (TH − TC ) q4 = 0
  • 121. Vb • Four steps w1 = − nRTH ln • Isothermal expansion: a to b Va dU = 0 w1 = − q1 γ −1 γ −1 • Adiabatic expansion: b to c TH Vb = TLVc w2 = nCV (TL − TH ) q2 = 0 Vd • Isothermal compression: c to d w3 = −nRTL ln Vc dU = 0 w3 = −q3 • Adiabatic compression: d to a γ −1 γ −1 TH Va = TLVd w4 = nCV (TH − TC ) q4 = 0
  • 122. wcycle = w1 + w2 + w3 + w4 Vb V wcycle = − nRTH ln + nC v (TL − TH ) − nRTL ln d + nC v (TH − TL ) Va Vc Vb V wcycle = − nRTH ln − nRTL ln d Va Vc ∫ dU = 0 Vb Vd TH Vb γ −1 = TLVc γ −1 qcycle = nRTH ln + nRTH ln Va Vc TLVd γ −1 = TH Va γ −1 γ −1 γ −1 TH Vc Vd Vc Vd wcycle V V = nRTH ln a − nRTL ln d = γ −1 = γ −1 ∴ = TL Vb Va Vb Va Vb Vc Va wcycle = nR(TH − TL ) ln Vb
  • 123. W QC efficiency = ε = = 1− QH QH But, QH = q1 = -w1 And, Qc = q3 = -w3 Vb Vd TH Vb γ −1 = TLVc γ −1 w1 = −nRTH ln w3 = −nRTL ln Va Vc T V γ −1 = T V γ −1 L d H a dU = 0 dU = 0 TH Vc γ −1 Vd γ −1 Vc Vd = = ∴ = w1 = −q1 w3 = −q3 TL Vb γ −1 Va γ −1 Vb Va ε = 1 – │Qc│/ │QH│ = 1 – TLln (Vd/Vc)/ THln (Vb/Va) 1 – │Qc│/ │QH│ = 1 – TL/ TH │Qc│/ │QH│ = TL/ TH │Qc│/ │ TL │ = │QH│ / TH │Qc│/ │ TL │ – │QH│ / TH = 0 (here, Qc ≡ QL) qi ∂q ∑ =0 ⇒∫ =0 Thus, the term δq/T is a state function Ti T
  • 124. Carnot’s theorem tells us that no real engine can have an efficiency more than that of the Carnot engine. TH − TL T η= = 1− L TH TH qH − qL η= qH qH − qL TH − TL ∴ = qH TH qL TL qL TL 1− = 1− ⇒− + =0 qH TH qH TH Multiply by qH TL qL qH qH qL q − + = 0; = ⇒ = cons tan t TL TH TH TL T
  • 125. When the Carnot cycle is operating as a heat engine (going around clockwise), w < 0, so that -w > 0 and q > 0. Va wcycle = nR(TH − TL ) ln Vb − wcycle wcycle Efficiency, ε or η = = q1 q1 Va − nR(TH − TL ) ln Vb TH − TL TL η= = = 1− Vb TH TH nRTH ln Va • Efficiency of Carnot engine < 1 • No cycle can have an efficiency greater than a Carnot cycle • All reversible engines operates between same 2 temperatures have same efficiency
  • 126. Carnot Cycle (Ideal gas, All the steps are reversible) 1 (A to B) 2 (B to C) 3 (C to D) 4 (D to A) Total (A to A) W - nRThln(VB/V A) CV(T-T ) C h - nRT ln(VD/V C C) CV(T-T ) h C + nR(T – T) ln(V/V ) C h B A q + nRT ln(V/V ) h B A Zero + nRT ln(V/V ) C D C Zero + nR h – T) ln(V/V ) (T C B A DU Zero CV(T-T ) C h Zero CV(T-T ) h C Zero + nR ln(V A) B/V Zero + nR ln(V C) D/V Zero Zero (qrev/ T) A (pA, VA, Th) B (pB, VB, Th) γ −1 γ −1 γ −1 γ −1 γ −1 TV = const.; ThVB = TCVC ThVA = TCVD (pD, VD, TC) D C (pC, VC, TC) γ −1 γ −1 ⎛ VB ⎞ ⎛V ⎞ ⎛ VB ⎞ ⎛ VC ⎞ ⎜ ⎟ ⎜V ⎟ =⎜ C ⎟ ⎜V ⎟ ⎜ ⎟ =⎜ ⎟ ⎜V ⎟ ⎜V ⎟ Th > Tc ⎝ A⎠ ⎝ D⎠ ⎝ A⎠ ⎝ D⎠ ln (VD / VC ) = − ln (VB / VA )
  • 127. Entropy • Our study of the Carnot cycle showed that over the cycle q/T = 0. • Since any reversible cycle can be approximated by a series of Carnot cycles, we expect that the integral of dQ/T along the closed path of the cycle = 0. • One consequence is that the integral of dQ/T between a and b is independent of the path. • The quantity dQ/T is called the entropy dS. • The entropy difference between a and b is thus path independent, and entropy is a state variable.
  • 128. Entropy • Entropy is a state variable, but Q and W are not state variables since they depend on the path used to get from a to b. • For a reversible process, the change in the entropy of the engine is opposite to the change in entropy of the environment that provides the heat required (or absorbs the heat generated). The net change in the total entropy = 0. • For an irreversible process, the net change in the total entropy will be larger than 0.
  • 129. Entropy : – Is a measure of the disorderness of a system. – In a reversible thermodynamic process, entropy of a system is related the change in the extent to which energy is dispersed in a disorderly manner, which in turn depends on the amount of energy transferred as heat (as heat stimulates motion) to the surroundings. – Is a measure of the energy in a system or process that is unavailable to do work. • For a process occurring at constant temperature (an isothermal process): qrev = the heat that is transferred when the process is carried out reversibly at a constant temperature. T = temperature at which the heat is transferred (in Kelvin).
  • 130. Second Law of Thermodynamics Entropy of the universe (i.e., Total Entropy): • Does not change for reversible processes • Increases for spontaneous processes. • But, entropy can decrease for individual systems Reversible (ideal): Irreversible (real, spontaneous):
  • 131. 2nd law of thermodynamics dSUniv = dSsys + dSsurr > 0 Spontaneous process dSUniv = dSsys + dSsurr = 0 Equilibrium process dSUniv = dSsys + dSsurr < 0 Impossible process For any process “=“ for reversible, equilibrium dSsys + dSsurr ≥ 0 “>” spontaneous (irreversible) (real) all spontaneous processes are irreversible
  • 132. Example • Show the Carnot cycle on a T-S diagram and identify the heat transfer at both the high and low temperatures, and the work output from the cycle. • 1-2, reversible isothermal heat transfer T 1 2 QH = ∫TdS = TH(S2-S1) area 1-2-B-A TH • 2-3, reversible, adiabatic expansion isentropic process, S=constant (S2=S3) TL 4 3 • 3-4, reversible isothermal heat transfer QL = ∫TdS = TL(S4-S3), area 3-4-A-B A B S1=S4 S2=S3 S • 4-1, reversible, adiabatic compression isentropic process, S1=S4 • Net work Wnet = QH - QL, the area enclosed by 1-2-3-4, the shaded area
  • 133. Efficiency of an heat engine TH Consider a Carnot heat engine. 1.What fraction of the total heat transferred Qh Qh to engine is converted into work in the cycle? Wby QC a. ∆T/TH b. ∆T/TC c. TC/TH TC 2. What is efficiency of reverse engine (refrigerator)? Coefficient of Performance a. QC / W b. Tc/ (TH-TC) c. 1-TH/TC 3. When can the heat engine convert the absorbed heat into work completely?. a. At TH = -273 ˚C b. At Tc = O ˚C c. when TC =-273 ˚C
  • 134. A Carnot heat engine receives 500 kJ of heat per cycle from a high- temperature heat reservoir at 652oC and rejects heat to a low- temperature heat reservoir at 30oC. Determine (a) The thermal efficiency of this Carnot engine. (b) The amount of heat rejected to the low-temperature heat reservoir. a. TL η th , rev = 1 − TH TH = 652oC ( 30 + 273) K = 1− ( 652 + 273) K QH = 0.672 or 67.2% WOUT HE QL QL T b. = L TL = 30oC QH TH ( 30 + 273) K = = 0.328 ( 652 + 273) K Q L = 500 kJ ( 0.328) = 164 kJ
  • 135. Suppose a mole of a diatomic gas, such as O2, is compressed adiabatically so the final volume is half the initial volume. The starting state is V = 1 liter, T = 300 K. What are the final temperature and pressure? p iV i γ = p f V fγ Equation relating p,V for adiabatic process in α- ideal gas γ = 7/2 = 1 .4 γ is the ratio of Cp/CV for diatomic gas in this case 5/2 γ ⎛V ⎞ Solve for pf from first equation pf = pi ⎜ i ⎟ ⎜V ⎟ ⎝ f ⎠ γ Substitute for pi nRT i ⎛ V i ⎜ ⎞ ⎟ = Vi ⎜ V f ⎝ ⎟ ⎠ = 6 . 57 x10 6 Pa p fV f Use ideal gas law to calculate final temperature Tf = nR OR use the equation relating T,V for an adiabatic = 395 K process to get the final temperature (α = 5/2 for T i α V i = T fα V f diatomic gas) 1 ⎛V ⎞ α T f = Ti ⎜ i ⎟ Solve for Tf ⎜V ⎟ ⎝ f ⎠ = 395 K
  • 136. Entropy change in heat engine Th Consider a Carnot heat engine. 1. What is the sign of the entropy change of Q the hot reservoir during one cycle? Wby h a. ΔSh < 0 b. ΔSh = 0 c. ΔSh > 0 QC Because energy is flowing out of the hot reservoir, its Tc entropy (the number of microstates) is decreasing. 2. What is the sign of the entropy change of the cold reservoir? a. ΔSc < 0 b. ΔSc = 0 c. ΔSc > 0 Because energy is flowing into the cold reservoir, it’s entropy (number of microstates) is increasing. 3. Compare the magnitudes of the two changes. a. |ΔSc| < |ΔSh| b. |ΔSc| = |ΔSh| c. |ΔSc| > |ΔSh|