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MAPPING ENERGY STATES ON
CU(775) USING ANGLE-RESOLVED
TWO-PHOTON PHOTOEMISSION
Advisor: Prof. R.M. Osgood, Prof. K. Bergman
Kevin Knox, Jerry Dadap
Speaker: Po-Chun Yeh
OUTLINE
Goal –Understanding the band structure of
Cu.
Understanding of Cu Band
structure - bulk state
Simulatio
n
AR2PP
E
Ultra-fast
Laser
with
OPA-SHG
A. ANGLE RESOLVED TWO PHOTON
PHOTOEMISSION - ENVIRONMENT
OUR SOURCE: TI:SAPHIRE LASER
Red and Infrared light in the range from 650 to 1100 nm.
Power: 0.5~1.5 Watt.
490 – 660 nm
• 2 fs pulse length
• 250 kHz repetition rate
• Bandwidth ~ 5 nm, 100 meV
• Pulse energy ~ 10 nJ
• Peak power ~ 100 kW
Ti:S Oscillator
Regen Amplifier
With CPA
Optical Parametric
Amplifier
800 nm
245 – 330 nm
(3.75 – 5 eV)
Second Harmonic
Generation
q
e–
UHV
Energy
Analyzer
Pulse Counter
MCP
Sample
q
e–
UHV
Energy
Analyzer
Pulse Counter
MCP
Sample
TECHNIQUE: 2PPE USING OPA-SHG
 Excellent tunability 3.75- 5.0 eV
 Capable of selecting transitions 
Resonances
 High pulse power, large e/pulse especially
for h ~   space charge effects
 Stability
 Reduced energy resolution for fs pulses
It ‘aint easy!
D. Strickland and G. Mourou, Opt. Commun. 1985
Stretcher Amplifier Compressor
Why CPA is important?
Direct amplification of ultrafast pulses
can damage Ti:S crystal and cause
self-phase modulation and gain
saturation
Amplified peak power ~ 50 MW
Peak focused intensity ~ 10 TW/cm2
CHIRPED PULSE AMPLIFICATION (CPA)
A. Ti:S Oscillator
Nd:YVO4 pump
C. Ti:S Regen Amp
B. Expander/Compressor
D. Optical
Parametric
Amplifier
Nd:YVO4 pump
E C Out
LAYOUT
CW 532 nm pump
5W from Nd:YVO4
100 fs, 100 MHz
10 nJ, 800 nm
OUTPUT TO
EXPANDER
A. SCHEMATIC OF TI:S OSCILLATOR
Ti: Sapphire
Crystal
Pumping cause population inversion -> Laser
FROM
OSCILLATOR
TO
REGEN
FROM
REGEN
TO
OPA
GRATING
GRATING
B. EXPANDER/COMPRESSOR LAYOUT
EXPANDER
COMPRESSOR
GATE
INPUT FROM EXPANDER
OUTPUT TO COMPRESSOR
10W PUMP
Nd:YVO4
C. SCHEMATIC OF TI:S REGEN AMPLIFIER
1 2 1 2
1: Inject Seed
Pulse
2: Eject
Amplified Pulse
Population
Inversion –
Gain > Loss
~25 rounds
in resonator
- AMPLIFY
800 nm
800 nm
400 nm
White light
Signal 480-700 nm
Idler 930-2300 nm
D.OPA OPTICAL SCHEMATIC
Split
pulse
Halves
λ,
Double
s
Energy
Combine,
Amplify
Specific Freq.
Gives us a tunable, high
intensity/resolution, ultra-short UV
pulse as input photons.
B. AR2PPE
THEORY AND EXPERIMENT
EF
E
k||0
Evac
Observed Electron Distribution Curve
Unoccupied
State
Occupied
Surface State
Resonant
Excitation
(ii) (iii) (i)
•2PPE allows population and probing
of normally unoccupied states.
i. Excited state electron
scattered into image state.
ii. Resonantly excited from
the surface state to the
image state.
iii. Direct absorption of two
photons.
TWO-PHOTON PHOTOEMISSION
ANGLE-RESOLVED-2PPE SPECTROSCOPY
q
e–
UHVPulse Counter
Energy
Analyzer
MCP
Sample
Tunable femtosecond
UV source
3. Angle-Resolved
measurement &
Spherical-sector
energy analyzer
4. Electron counting
at high repetition rate
1. Sample prepared via
repeated sputtering &
annealing cycles.
2. Low Energy
Electron Diffraction
LEED Image
For stepped surfaces each state can have different reference planes.
[112]
[110]
[111]
CU(775)-STEPPED SURFACES
Cu
2cm
8.5 degree
(Side View)
COMPARISON:
2PPE FROM FLAT CU(111)
Resonant mapping of Cu(111)
surface state and n=1 state
Photoemission intensity vs. emission
angle and KE of emitted electrons.
Resonant
Peaks
Surface State
Emission
n=1 Image State
Emission
Surface state
n=1 image state
Cu (111)
Surface state
n=1 image state
2PPE FROM CU(775)
Resonant
Peaks
Resonant Mapping
Location of peaks – Measured KE,
2PPE Photon Energy yields map of
states
MEASUREMENT & RESULT
We can only measure Kinetic Energy and Number of output electrons!
Evac
EFermi
Evac
Energy(eV)
K

M
EL-GAP= 4.9 eV
Evac
EFermi
Evac
Energy(eV)
K

M
EL-GAP= 4.9 eV
Projection
C. BAND STRUCTURE SIMULATION
SIMULATION
Calculating:
 The impact of Cu(775) tilted surface.
 Possible energy states Cu(775) – Fortran 77
 Filtering the result using known Cu properties,
input conditions, and experiences.
Relation between K parallel
and Proper kinetic energy
is what we want to know
about!
STEP1 MODIFICATION OF TILTED SURFACE
K Parallel
K
Perpendicular
K
Tilted?
K’
CACULATION
 Define variable (R, n) for K parallel and K
perpendicular!
 Proof: Orthogonal Coordinates – Product
Rule
 Get tilted K(Kx, Ky, Kz)
Kx = Ky = (SQRT(3))/2 *1.74*R - 0.01*n*0.7/1.407
Kz = (SQRT(3))/2 *1.74*1.4*R + 0.01*n*1/1.407
R = Testing number from 0.100~0.900
n = +50 to -50
When R=0.5, |K| = 1.5 ± 0.5 / A (Amstrong), matching
the flat Cu(111) experimental range.
ENERGY STATES
 Band structure of Cu can be calculated using
tight-bonded potential model!
 Need values of K’ and characteristic parameters
of Cu, such as energy gaps, Fermi level,
effective mass, etc. (Papaconstantopoulos’s
book; papers)
0.0 0.2 0.4 0.6 0.8 1.0
0.0
0.5
1.0
1.5
2.0
2.5
3.0
3.5
4.0
YAxisTitle
XAxisTitle
0.0 0.1 0.2 0.3 0.4 0.5
0.0
0.5
1.0
1.5
2.0
2.5
3.0
3.5
4.0
YAxisTitle
XAxisTitle
0.0 0.1 0.2 0.3 0.4 0.5
0.0
0.5
1.0
1.5
2.0
2.5
3.0
3.5
4.0YAxisTitle
XAxisTitle
0.5 0.4 0.3 0.2 0.1 0.0
0.0
0.5
1.0
1.5
2.0
2.5
3.0
3.5
4.0
YAxisTitle
XAxisTitle
0.0 0.2 0.4 0.6 0.8 1.0
0.0
0.5
1.0
1.5
2.0
2.5
3.0
3.5
4.0
YAxisTitle
XAxisTitle
 X L  XKSD LWZ Q
CALCULATION OF ENERGY STATES
 Using the theory and parameters to build a
9x9 Matrix, solving the eigenvalues (≦9).
 Program on Fortran 77 (Was created by Dr.
Dimitrios and we modified it.)
Read in initial and final k values, Cu
parameters, and other settings.
Calculating the matrix on directions as
follows: Γ -> L, X -> W -> L -> K -> Γ -> K.
Call in IMSL numerical library to tri-
diagonalize and solve the matrix.
Output performance factor, eigenvectors
and eigenvalues.
Generate data for the 9 energy levels to
each set of k values. (~ 9000 data)
CALCULATE THE RIGHT RESULT
 If not interpreted and modified properly, the result
is useless.
Conditions:
 1. Transition happens between E7 & E6
 2. Cu work function: 4.9eV
 3. Proper energy shifting should make E7 > 0
and E6 < 0 while Zero Point Energy = Fermi
Energy
 4. Given Photon Energy hv
 5. 1st PPE: E7 – E6 = hv, error < 0.02 eV
 6. 2nd PPE: E7 + hv – Work Func. = Kinetic
Energy
In short, 2PPE happens between precise energy
states. Also, the energy of 1st PPE should lower
than work function; otherwise we will get the
wrong states.
PHOTON ENERGY DEPENDENCE
– THE BULK STATE
0
5
10
15
20
25
30
0.5
0.47
0.44
0.41
0.38
0.35
0.32
0.29
0.26
0.23
0.2
0.17
0.14
0.11
0.08
0.05
0.02
-0.01
-0.04
-0.07
-0.1
-0.13
-0.16
-0.19
-0.22
-0.25
-0.28
-0.31
-0.34
-0.37
-0.4
-0.43
-0.46
-0.49
ΔE(R=0.6)
ΔE(R=0.55)
ΔE(R=0.5)
ΔE(R=0.45)
ΔE(R=0.4)
ΔE(R=0.35)
ΔE(R=0.3)
ΔE(R=0.25)
ΔE(R=0.2)
ΔE(R=0.15)
0
2
4
6
8
10
12
0.5
0.47
0.44
0.41
0.38
0.35
0.32
0.29
0.26
0.23
0.2
0.17
0.14
0.11
0.08
0.05
0.02
-0.01
-0.04
-0.07
-0.1
-0.13
-0.16
-0.19
-0.22
-0.25
-0.28
-0.31
-0.34
-0.37
-0.4
-0.43
-0.46
-0.49
R=0.33
R=0.32
R=0.31
R=0.3
R=0.29
R=0.28
R=0.27
R=0.26
R=0.25
R=0.24
RESULT: E= 4.66EV
3.8
3.9
4
4.1
4.2
4.3
4.4
4.5
4.6
4.7
(0.3000) (0.2500) (0.2000) (0.1500) (0.1000) (0.0500) 0.0000
Ek
Ek
RESULT: E= 5.02EV
3.8
3.9
4
4.1
4.2
4.3
4.4
4.5
4.6
4.7
-0.3 -0.25 -0.2 -0.15 -0.1 -0.05 0
Ek
DISCUSSION
2 Good 2 Bad
 Slope and shape is pretty near!
 Built up a standard procedure to do
calculation fast.
 Energy shift problem.
 n all negative/positive – need further study.
FUTURE PLAN
 Need more data, especially with energies
close to boundary (work func.)
 Using higher photon energy.
 Different approach on the calculation (New
model, different length, etc.)
 Re-program it on other languages with a
more user-friendly interface.
REFERENCES
 Nonequilibrium Band Mapping of Unoccupied Bulk States Below the Vaccum
Level by Two-Photon Photoemission, by Zhaofeng Hao, J. I. Dadap, K. Knox, M.
Yilmaz, N. Zaki, P. D. Johnson, and R. M. Osgood. (Pending on PRL)
 Electronic structure of a Co-decorated vicinal Cu(775) surface: High-resolution
photoemission spectroscopy, by S.-C. Wang, M. B. Yilmaz, K. R. Knox, N. Zaki,
J. I. Dadap, T. Valla, P. D. Johnson, and R. M. Osgood, Phys. Rev. B 77, 115448
(2008).
 Scattering of Surface States at Step Edges in Nanostripe Arrays, by F. Schiller,
M. Ruiz-Dses, J. Cordon, and J. E. Ortega, Phy. Rev. Lett. 95, 066805 (2005).
 Observation of a one-dimensional state on stepped Cu(775), by X. J. Shen, H.
Kwak, D. Mocuta, A. M. Radojevic, S. Smadici, and R. M. Osgood, Phys. Rev. B
63, 165403 (2001).
 Surface electron motion near monatomic steps: Two-photon photoemission
studies on stepped Cu(111), by X. Y. Wang, X. J. Shen, and R. M. Osgood,
Phys. Rev. B 56, 7665 (1997).
 Book: S. Hufner, Photoelectron Specstropy, 3rd ed. (Springer, Berlin, 2003)
 Book: Hai-Lung Dai, Wilson Ho, Laser Spectroscopy and Photo-Chemistry on
Metal Surfaces. (World Scientific, 1995)
 Book: Harald Ibach, Hans Luth, Solid State Physics. (Springer, 1991)
~FIN~
Q&A time
Thank you for
your patience!
q
e–
UHV
Pulse Counter
Energy
Analyzer
MCP
Sample
Oscillator
YVO4 pump
egen Amp
B. Expander/Compressor
D. Optical
Parametric
Amplifier
YVO4 pump
E C Out
Copper (775) - an optics, 2PPE, and Bulk state simulation study

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Copper (775) - an optics, 2PPE, and Bulk state simulation study

  • 1. MAPPING ENERGY STATES ON CU(775) USING ANGLE-RESOLVED TWO-PHOTON PHOTOEMISSION Advisor: Prof. R.M. Osgood, Prof. K. Bergman Kevin Knox, Jerry Dadap Speaker: Po-Chun Yeh
  • 2. OUTLINE Goal –Understanding the band structure of Cu. Understanding of Cu Band structure - bulk state Simulatio n AR2PP E Ultra-fast Laser with OPA-SHG
  • 3. A. ANGLE RESOLVED TWO PHOTON PHOTOEMISSION - ENVIRONMENT
  • 4. OUR SOURCE: TI:SAPHIRE LASER Red and Infrared light in the range from 650 to 1100 nm. Power: 0.5~1.5 Watt.
  • 5. 490 – 660 nm • 2 fs pulse length • 250 kHz repetition rate • Bandwidth ~ 5 nm, 100 meV • Pulse energy ~ 10 nJ • Peak power ~ 100 kW Ti:S Oscillator Regen Amplifier With CPA Optical Parametric Amplifier 800 nm 245 – 330 nm (3.75 – 5 eV) Second Harmonic Generation q e– UHV Energy Analyzer Pulse Counter MCP Sample q e– UHV Energy Analyzer Pulse Counter MCP Sample TECHNIQUE: 2PPE USING OPA-SHG  Excellent tunability 3.75- 5.0 eV  Capable of selecting transitions  Resonances  High pulse power, large e/pulse especially for h ~   space charge effects  Stability  Reduced energy resolution for fs pulses It ‘aint easy!
  • 6. D. Strickland and G. Mourou, Opt. Commun. 1985 Stretcher Amplifier Compressor Why CPA is important? Direct amplification of ultrafast pulses can damage Ti:S crystal and cause self-phase modulation and gain saturation Amplified peak power ~ 50 MW Peak focused intensity ~ 10 TW/cm2 CHIRPED PULSE AMPLIFICATION (CPA)
  • 7. A. Ti:S Oscillator Nd:YVO4 pump C. Ti:S Regen Amp B. Expander/Compressor D. Optical Parametric Amplifier Nd:YVO4 pump E C Out LAYOUT
  • 8. CW 532 nm pump 5W from Nd:YVO4 100 fs, 100 MHz 10 nJ, 800 nm OUTPUT TO EXPANDER A. SCHEMATIC OF TI:S OSCILLATOR Ti: Sapphire Crystal Pumping cause population inversion -> Laser
  • 10. GATE INPUT FROM EXPANDER OUTPUT TO COMPRESSOR 10W PUMP Nd:YVO4 C. SCHEMATIC OF TI:S REGEN AMPLIFIER 1 2 1 2 1: Inject Seed Pulse 2: Eject Amplified Pulse Population Inversion – Gain > Loss ~25 rounds in resonator - AMPLIFY
  • 11. 800 nm 800 nm 400 nm White light Signal 480-700 nm Idler 930-2300 nm D.OPA OPTICAL SCHEMATIC Split pulse Halves λ, Double s Energy Combine, Amplify Specific Freq. Gives us a tunable, high intensity/resolution, ultra-short UV pulse as input photons.
  • 12. B. AR2PPE THEORY AND EXPERIMENT
  • 13. EF E k||0 Evac Observed Electron Distribution Curve Unoccupied State Occupied Surface State Resonant Excitation (ii) (iii) (i) •2PPE allows population and probing of normally unoccupied states. i. Excited state electron scattered into image state. ii. Resonantly excited from the surface state to the image state. iii. Direct absorption of two photons. TWO-PHOTON PHOTOEMISSION
  • 14. ANGLE-RESOLVED-2PPE SPECTROSCOPY q e– UHVPulse Counter Energy Analyzer MCP Sample Tunable femtosecond UV source 3. Angle-Resolved measurement & Spherical-sector energy analyzer 4. Electron counting at high repetition rate 1. Sample prepared via repeated sputtering & annealing cycles. 2. Low Energy Electron Diffraction LEED Image
  • 15. For stepped surfaces each state can have different reference planes. [112] [110] [111] CU(775)-STEPPED SURFACES Cu 2cm 8.5 degree (Side View)
  • 16. COMPARISON: 2PPE FROM FLAT CU(111) Resonant mapping of Cu(111) surface state and n=1 state Photoemission intensity vs. emission angle and KE of emitted electrons. Resonant Peaks Surface State Emission n=1 Image State Emission Surface state n=1 image state Cu (111)
  • 17. Surface state n=1 image state 2PPE FROM CU(775) Resonant Peaks Resonant Mapping Location of peaks – Measured KE, 2PPE Photon Energy yields map of states
  • 18. MEASUREMENT & RESULT We can only measure Kinetic Energy and Number of output electrons! Evac EFermi Evac Energy(eV) K  M EL-GAP= 4.9 eV Evac EFermi Evac Energy(eV) K  M EL-GAP= 4.9 eV Projection
  • 19. C. BAND STRUCTURE SIMULATION
  • 20. SIMULATION Calculating:  The impact of Cu(775) tilted surface.  Possible energy states Cu(775) – Fortran 77  Filtering the result using known Cu properties, input conditions, and experiences. Relation between K parallel and Proper kinetic energy is what we want to know about!
  • 21. STEP1 MODIFICATION OF TILTED SURFACE K Parallel K Perpendicular K Tilted? K’
  • 22. CACULATION  Define variable (R, n) for K parallel and K perpendicular!  Proof: Orthogonal Coordinates – Product Rule  Get tilted K(Kx, Ky, Kz) Kx = Ky = (SQRT(3))/2 *1.74*R - 0.01*n*0.7/1.407 Kz = (SQRT(3))/2 *1.74*1.4*R + 0.01*n*1/1.407 R = Testing number from 0.100~0.900 n = +50 to -50 When R=0.5, |K| = 1.5 ± 0.5 / A (Amstrong), matching the flat Cu(111) experimental range.
  • 23. ENERGY STATES  Band structure of Cu can be calculated using tight-bonded potential model!  Need values of K’ and characteristic parameters of Cu, such as energy gaps, Fermi level, effective mass, etc. (Papaconstantopoulos’s book; papers) 0.0 0.2 0.4 0.6 0.8 1.0 0.0 0.5 1.0 1.5 2.0 2.5 3.0 3.5 4.0 YAxisTitle XAxisTitle 0.0 0.1 0.2 0.3 0.4 0.5 0.0 0.5 1.0 1.5 2.0 2.5 3.0 3.5 4.0 YAxisTitle XAxisTitle 0.0 0.1 0.2 0.3 0.4 0.5 0.0 0.5 1.0 1.5 2.0 2.5 3.0 3.5 4.0YAxisTitle XAxisTitle 0.5 0.4 0.3 0.2 0.1 0.0 0.0 0.5 1.0 1.5 2.0 2.5 3.0 3.5 4.0 YAxisTitle XAxisTitle 0.0 0.2 0.4 0.6 0.8 1.0 0.0 0.5 1.0 1.5 2.0 2.5 3.0 3.5 4.0 YAxisTitle XAxisTitle  X L  XKSD LWZ Q
  • 24. CALCULATION OF ENERGY STATES  Using the theory and parameters to build a 9x9 Matrix, solving the eigenvalues (≦9).  Program on Fortran 77 (Was created by Dr. Dimitrios and we modified it.) Read in initial and final k values, Cu parameters, and other settings. Calculating the matrix on directions as follows: Γ -> L, X -> W -> L -> K -> Γ -> K. Call in IMSL numerical library to tri- diagonalize and solve the matrix. Output performance factor, eigenvectors and eigenvalues. Generate data for the 9 energy levels to each set of k values. (~ 9000 data)
  • 25. CALCULATE THE RIGHT RESULT  If not interpreted and modified properly, the result is useless. Conditions:  1. Transition happens between E7 & E6  2. Cu work function: 4.9eV  3. Proper energy shifting should make E7 > 0 and E6 < 0 while Zero Point Energy = Fermi Energy  4. Given Photon Energy hv  5. 1st PPE: E7 – E6 = hv, error < 0.02 eV  6. 2nd PPE: E7 + hv – Work Func. = Kinetic Energy In short, 2PPE happens between precise energy states. Also, the energy of 1st PPE should lower than work function; otherwise we will get the wrong states.
  • 26. PHOTON ENERGY DEPENDENCE – THE BULK STATE 0 5 10 15 20 25 30 0.5 0.47 0.44 0.41 0.38 0.35 0.32 0.29 0.26 0.23 0.2 0.17 0.14 0.11 0.08 0.05 0.02 -0.01 -0.04 -0.07 -0.1 -0.13 -0.16 -0.19 -0.22 -0.25 -0.28 -0.31 -0.34 -0.37 -0.4 -0.43 -0.46 -0.49 ΔE(R=0.6) ΔE(R=0.55) ΔE(R=0.5) ΔE(R=0.45) ΔE(R=0.4) ΔE(R=0.35) ΔE(R=0.3) ΔE(R=0.25) ΔE(R=0.2) ΔE(R=0.15) 0 2 4 6 8 10 12 0.5 0.47 0.44 0.41 0.38 0.35 0.32 0.29 0.26 0.23 0.2 0.17 0.14 0.11 0.08 0.05 0.02 -0.01 -0.04 -0.07 -0.1 -0.13 -0.16 -0.19 -0.22 -0.25 -0.28 -0.31 -0.34 -0.37 -0.4 -0.43 -0.46 -0.49 R=0.33 R=0.32 R=0.31 R=0.3 R=0.29 R=0.28 R=0.27 R=0.26 R=0.25 R=0.24
  • 27. RESULT: E= 4.66EV 3.8 3.9 4 4.1 4.2 4.3 4.4 4.5 4.6 4.7 (0.3000) (0.2500) (0.2000) (0.1500) (0.1000) (0.0500) 0.0000 Ek Ek
  • 29. DISCUSSION 2 Good 2 Bad  Slope and shape is pretty near!  Built up a standard procedure to do calculation fast.  Energy shift problem.  n all negative/positive – need further study.
  • 30. FUTURE PLAN  Need more data, especially with energies close to boundary (work func.)  Using higher photon energy.  Different approach on the calculation (New model, different length, etc.)  Re-program it on other languages with a more user-friendly interface.
  • 31. REFERENCES  Nonequilibrium Band Mapping of Unoccupied Bulk States Below the Vaccum Level by Two-Photon Photoemission, by Zhaofeng Hao, J. I. Dadap, K. Knox, M. Yilmaz, N. Zaki, P. D. Johnson, and R. M. Osgood. (Pending on PRL)  Electronic structure of a Co-decorated vicinal Cu(775) surface: High-resolution photoemission spectroscopy, by S.-C. Wang, M. B. Yilmaz, K. R. Knox, N. Zaki, J. I. Dadap, T. Valla, P. D. Johnson, and R. M. Osgood, Phys. Rev. B 77, 115448 (2008).  Scattering of Surface States at Step Edges in Nanostripe Arrays, by F. Schiller, M. Ruiz-Dses, J. Cordon, and J. E. Ortega, Phy. Rev. Lett. 95, 066805 (2005).  Observation of a one-dimensional state on stepped Cu(775), by X. J. Shen, H. Kwak, D. Mocuta, A. M. Radojevic, S. Smadici, and R. M. Osgood, Phys. Rev. B 63, 165403 (2001).  Surface electron motion near monatomic steps: Two-photon photoemission studies on stepped Cu(111), by X. Y. Wang, X. J. Shen, and R. M. Osgood, Phys. Rev. B 56, 7665 (1997).  Book: S. Hufner, Photoelectron Specstropy, 3rd ed. (Springer, Berlin, 2003)  Book: Hai-Lung Dai, Wilson Ho, Laser Spectroscopy and Photo-Chemistry on Metal Surfaces. (World Scientific, 1995)  Book: Harald Ibach, Hans Luth, Solid State Physics. (Springer, 1991)
  • 32. ~FIN~ Q&A time Thank you for your patience!
  • 33. q e– UHV Pulse Counter Energy Analyzer MCP Sample Oscillator YVO4 pump egen Amp B. Expander/Compressor D. Optical Parametric Amplifier YVO4 pump E C Out