Formation of low mass protostars and their circumstellar disks
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Princeton conference Equivalent Theories in Physics and Metaphysics
1. Duality and Emergent Gravity
in AdS/CFT
Sebastian de Haro
University of Amsterdam and University of Cambridge
Equivalent Theories in Science and Metaphysics
Princeton, 21 March 2015
2. Motivating thoughts
โขDuality and emergence of space-time have been a
strong focus in quantum gravity and string theory
research in recent years
โขThe notion of โemergenceโ of space-time and/or
gravity is often attached to the existence of a
โdualityโ
3. Motivating thoughts
โข An argument along the following lines is
often made:
a) Theory F (โfundamentalโ) and theory G
(โgravityโ) are dual to one another
b) Theory F does not contain gravity (and/or
space-time) whereas theory G does
c) Therefore space-time (and/or gravity)
emerges in theory G. Theory F is to be
regarded as more fundamental
4. โข But this argument is problematic: it replaces โdualityโ
by โemergenceโ.
โข Duality is a symmetric relation, whereas emergence is
not symmetric
โข We need to explain what breaks the symmetry
โข Emergence of space-time requires more than simply
โthe space-time being dual to something that is not
spatio-temporalโ
โข It might lead to bad heuristics for constructing new
theories, e.g. when the argument is taken as a reason
not to pursue theory G but to just work on theory F
โข I will discuss the notions of duality and emergence in
holographic scenarios, in particular AdS/CFT
โข I will only discuss the possible emergence of gravity
together with one, spatial dimension.
โข This is a non-trivial task: for obtaining the right classical
dynamics for the metric is hard!
5. Introduction: โt Hooftโs Holographic Hypothesis
โข The total number of degrees of freedom, ๐, in a region of space-time
containing a black hole, is:
๐ =
๐
log 2
=
๐ด
4๐บlog 2
โข Hence, โwe can represent all that happens inside [a volume] by
degrees of freedom on the surfaceโ
โข โThis suggests that quantum gravity should be described entirely by a
topological quantum field theory, in which all degrees of freedom can
be projected on to the boundaryโ
โข โWe suspect that there simply are no more degrees of freedom to
talk about than the ones one can draw on a surface [in bit/Planck
length2]. The situation can be compared with a hologram of a three
dimensional image on a two dimensional surfaceโ
6. Introduction: โt Hooftโs Holographic Hypothesis
โข The observables โcan best be described as ifโ they were Boolean
variables on a lattice, which suggests that the description on the
surface only serves as one possible representation
โข Nevertheless, 't Hooft's account more often assumes that the
fundamental ontology is the one of the degrees of freedom that scale
with the space-time's boundary. He argued that quantum gravity
theories that are formulated in a four dimensional space-time, and
that one would normally expect to have a number of degrees of
freedom that scales with the volume, must be โinfinitely correlated"
at the Planck scale
โข The explanatory arrow here clearly goes from surface to bulk, with
the plausible implication that the surface theory should be taken as
more basic than the theory of the enclosed volume
โข There is no indication that a notion of emergence is relevant here
7. Introduction: โt Hooftโs Holographic Hypothesis
โข โt Hooftโs paper wavers between boundary and bulk as fundamental
ontologies
โข There is an interpretative tension here, that resurfaces in other
contexts where there are dualities
8. Philosophical concerns regarding
holographic dualities:
โขCan one decide which side of the duality is
more fundamental?
โขIs one facing emergence of space, time,
and/or gravity?
9. Plan
โขDuality:
โข Introduction to AdS/CFT
โข Duality
โข Renormalization group
โข Diffeomorphism invariance and background
independence
โข Interpretation
โขEmergence
10. Geometry of AdS ๐ท
โข Hyperboloid in ๐ท + 1 dimensions:
โ๐0
2
โ ๐ ๐ท
2
+
๐=1
๐ทโ1
๐๐
2
= โโ2
โข Constraint can be solved introducing ๐ท coordinates:
๐0 = โ cosh ๐ cos ๐
๐ ๐ท = โ cosh ๐ sin ๐
๐๐ = โ sinh ๐ ฮฉ๐ ๐ = 1, โฆ , ๐ = ๐ท โ 1 , ฮฉ๐ = unit vector
โข Leading to: d๐ 2
= โ2
โ cosh2
๐ d๐2
+ d๐2
+ sinh2
๐ dฮฉ ๐ทโ2
2
โข Symmetry group SO 2, ๐ apparent from the construction
โข Riemann tensor in terms of the metric (negative curvature):
๐ ๐๐๐๐ = โ
1
โ2
๐ ๐๐ ๐ ๐๐ โ ๐ ๐๐ ๐ ๐๐
๐๐
๐0
๐ ๐ท
โ
11. Geometry of AdS ๐ท
โข Useful choice of local coordinates:
d๐ 2
=
โ2
๐2 d๐2
+ ๐๐๐ d๐ฅ ๐
d๐ฅ ๐
, ๐ = 1, โฆ , ๐ = ๐ท โ 1
โข ๐๐๐ = flat metric (Lorentzian or Euclidean signature)
โข Can be generalised to (AL)AdS:
d๐ 2
=
โ2
๐2 d๐2
+ ๐๐๐ ๐, ๐ฅ d๐ฅ ๐
d๐ฅ ๐
๐๐๐ ๐, ๐ฅ = ๐ 0 ๐๐ ๐ฅ + ๐ ๐ 1 ๐๐ ๐ฅ + ๐2 ๐ 2 ๐๐ ๐ฅ + โฏ
โข Einsteinโs equations now reduce to algebraic relations between
๐ ๐ ๐ฅ ๐ โ 0, ๐ and ๐ 0 ๐ฅ , ๐ ๐ ๐ฅ
12. Adding Matter
โข Matter field ๐ ๐, ๐ฅ (for simplicity, take ๐ = 0), solve KG equation
coupled to gravity:
๐ ๐, ๐ฅ = ๐ 0 ๐ฅ + ๐ ๐ 1 ๐ฅ + โฏ + ๐ ๐
๐ ๐ ๐ฅ + โฏ
โข Again, ๐ 0 ๐ฅ and ๐ ๐ ๐ฅ are the boundary conditions and all other
coefficients ๐ ๐ ๐ฅ are given in terms of them (and the metric)
14. Example: AdS5 ร ๐5
= SU ๐ SYM
AdS5 ร ๐5
โข Type IIB string theory
โข Limit of small curvature:
supergravity (Einsteinโs theory +
specific matter fields)
โข Symmetry of AdS: diffeoโs that
preserve form of the metric
generate conformal
transformations on the bdy
โข Symmetry of ๐5
SU ๐ SYM
โข Supersymmetric Yang-Mills
theory with gauge group SU(๐)
โข Limit of weak coupling: โt Hooft
limit (planar diagrams)
โข Classical conformal invariance of
the theory
โข Symmetry of the 6 scalar fields
โข Limits are incompatible (weak/strong coupling duality: useful!)
โข Only gauge invariant quantities (operators) can be compared
โข Symmetry:
SO 2,4 ร SO 6
15. What is a Duality? (Butterfield 2014)
โข Regard a theory as a triple ๐ฎ, ๐ช, ๐ท
โข ๐ฎ = states (in Hilbert space)
โข ๐ช = operators (self-adjoint, renormalizable, invariant under symmetries)
โข ๐ท = dynamics (given by e.g. Lagrangian and integration measure)
โข A duality is an isomorphism between two theories ๐ฎ๐ด, ๐ช ๐ด, ๐ท๐ด and
๐ฎ ๐ต, ๐ช ๐ต, ๐ท ๐ต .
โข There exist bijections:
โข ๐ ๐ฎ: ๐ฎ๐ด โ ๐ฎ ๐ต,
โข ๐ ๐ช: ๐ช ๐ด โ ๐ช ๐ต
and pairings (vevs) ๐, ๐ ๐ด such that:
๐, ๐ ๐ด = ๐ ๐ช ๐ , ๐ ๐ฎ ๐ ๐ต โ๐ โ ๐ช ๐ด, ๐ โ ๐ฎ๐ด
17. AdS/CFT Duality
โข AdS/CFT can be described this way:
โข Normalizable modes correspond to vevs of operators (choice of state)
โข Fields correspond to operators
โข Boundary conditions (non-normalizable modes) correspond to couplings
โข Dynamics otherwise different (different Lagrangian, different dimensions!)
โข Two salient points of :
โข Part of the dynamics now also agrees (couplings in the Lagrangian vs.
boundary conditions). This is the case in any duality that involves parameters
that are not operators, e.g. T-duality (๐ โ 1/๐ ), electric-magnetic duality
(๐ โ 1/๐)
โข It is also more general: while ๐ฎ, ๐ช, ๐ท are a priori fixed, ๐ can be varied at
will. Thus we have a multidimensional space of theories
โข Dualities of this type are not isomorphisms between two given
theories, but between two sets of theories
๐ฎ
๐ช
๐
๐ท
๐, ๐ ๐ ,๐ท ๐ด
= ๐ ๐ช ๐ , ๐ ๐ฎ ๐ {๐ ๐(๐)} ,๐ท ๐ต
18. AdS/CFT Duality (Continued)
โขString theory in (AL)AdS space = QFT on boundary
โขFormula 1 is generated by:
๐string ๐ 0 =
๐ 0,๐ฅ =๐ 0 ๐ฅ
๐๐ ๐โ๐ ๐
= exp d ๐
๐ฅ ๐ 0 ๐ฅ ๐ช ๐ฅ
CFT
โขThe correlation functions of all operators match
โขPhysical equivalence, mathematical structure different
โขLarge distance โ high energy divergences 2
โขStrictly speaking, the AdS/CFT correspondence has the
status of a โconjectureโ, though there is massive evidence
for it (and it is usually called a โcorrespondenceโ:
compare e.g. Fermatโs last โtheoremโ before it was
proven!)
(1โฒ)
๐ ๐ต = ๐ ๐ ๐ ๐ด
19. Renormalization Group
โข Radial integration: โข Wilsonian renormalization:
ฮ๐ฮ0
๐
integrate out
New cutoff ๐ฮ
rescale ๐ฮ โ ฮ until ๐ โ 0
AdS ๐
๐AdS ๐ ๐AdS ๐
new boundary condition
integrate out
IR cutoff ๐ in AdS โ UV cutoff ฮ in QFT(2) ๐ ๐ต = ๐ ๐ ๐ ๐ด
20. Conditions for AdS/CFT Duality
โข What could lead to the failure of AdS/CFT as a duality?
โข Two conditions must be met for this bijection to exist. The observable
structures of these theories should be:
i. Complete (sub-) structures of observables, i.e. no other observables can
be written down than (1): this structure of observables contains what the
theories regard to be โphysicalโ independently on each side of the duality.
ii. Identical, i.e. the (sub-) structures of observables are identical to each
other.
๏If ii. is not met, we can have a weaker form of the conjecture: a relation that is
non-exact. For instance, if the duality holds only in some particular regime of the
coupling constants
โข There are no good reasons to believe that i. fails.
โข Whether ii. is met is still open, but all available evidence indicates that it is
satisfied, including some non-perturbative tests. However: see later
21. Remarks on Background Independence
โข Theories of gravity are usually required to be โbackground independentโ. In
Einsteinโs theory of relativity, the metric is a dynamical quantity, determined
from the equations of motion rather than being fixed from the outset
โข The concept of โbackground independenceโ does not have a fixed meaning,
see Belot (2011)
โข Here I will adopt a โminimalist approachโ: a theory is background independent
if it is generally covariant and its formulation does not make reference to a
background/fixed metric. In particular, the metric is determined dynamically
from the equations of motion
โข In this minimalist sense, classical gravity in AdS is fully background
independent: Einsteinโs equations with negative cosmological constant
โข Quantum corrections do not change this conclusion: they appear perturbatively as
covariant higher-order corrections to Einsteinโs theory
โข Could background independence be broken by the asymptotic form of the
metric?
โข This is just a choice of boundary condition. The equations of motion do not determine
them: they need to be specified additionally (de Haro et al. 2001)
โข But this is not a restriction on the class of solutions considered; as in classical mechanics,
the laws (specifically: the equations of motion) simply do not contain the informtion
about the boundary/initial conditions
โข Boundary conditions do not need to preserve the symmetries of the laws. Thus this does
not seem a case of lack of background independence of the theory. At most, it may lead
to spontaneous breaking of the symmetry in the sense of a choice of a particular solution
โข Hence, the background independence of the theory is well established
22. Diffeomorphism Invariance of (1โ)
โข I have discussed background independence of the equations of
motion. What about the observables?
โข Partition function (1โ):
โข It depends on the boundary conditions on the metric (as do the classical
solutions)
โข It is diffeomorphism invariant, for those diffeomorphisms that preserve the
asymptotic form of the metric
โข Other observables obtained by taking derivatives of (1): they
transform as tensors under these diffeomorphisms. These
observables are covariant, for odd d (=boundary dimension):
โข For odd ๐:
โข Invariance/covariance holds
โข For even ๐:
โข Bulk diffeomorphisms that yield conformal transformations of the boundary
metric are broken due to IR divergences (holographic Weyl anomaly). Is this
bad?
๐string ๐ฮ โ๐
๐ ๐, ๐ฅ
๐=0
= ๐ 0 ๐ฅ = ๐ d ๐ ๐ฅ ๐ 0 ๐ฅ ๐ช ๐ฅ
CFT
(1โฒ)
23. Diffeomorphism Invariance (even ๐)
โข The breaking of diffeomorphism invariance exactly mirrors the
breaking of conformal invariance by quantum effects in the CFT
โข The partition function now depends on the representative of the
conformal structure picked for regularization
โข The observables (1โ) such as the stress-tensor no longer transform
covariantly, but pick up an anomalous term
โข Anomalies are usually quantum effects, proportional to โ. Here,
the anomaly is (inversely) proportional to Newtonโs constant ๐บ
โข The anomaly is robust: it is fully non-linear and it does not rely on
classical approximations
โข This anomaly does not lead to any inconsistencies because the
metric is not dynamical in the CFT
24. Philosophical Questions
โขIs one side of the duality more fundamental?
โข If QFT more fundamental, space-time could be โemergentโ
โข If the duality is only approximate: room for emergence
(e.g. thermodynamics vs. atomic theory)
โข If duality holds good: one-to-one relation between the
values of physical quantities. In this case we have to
give the duality a physical interpretation
25. Interpretation
โขExternal view: meaning of observables is externally
fixed. Duality relates different physical quantities
โข No empirical equivalence, numbers correspond to
different physical quantities
โข The symmetry of the terms related by duality is broken by
the different physical interpretation given to the symbols
โข Example: ๐ fixed by the interpretation to mean โradial
distanceโ in the bulk theory. In the boundary theory, the
corresponding symbol is fixed to mean โrenormalization
group scaleโ. The two symbols clearly describe different
physical quantities. More generally, the two theories
describe different physics hence are not empirically
equivalent
โข Only one of the two sides provides a correct
interpretation of empirical reality
26. Interpretation
โขInternal point of view:
โข The meaning of the symbols is not fixed beforehand
โข There is only one set of observables that is described by
the two theories. The two descriptions are equivalent. No
devisable experiment could tell one from the other (each
observation can be reinterpreted in the โdualโ variables)
โข Cannot decide which description is superior. One
formulation may be superior on practical grounds (e.g.
computational simplicity in a particular regime)
โข On this formulation we would normally say that we have
two formulations of one theory, not two different
theories
27. Interpretation
โขThe internal point of view seems more natural for
theories of the whole world
โขEven if one views a theory as a partial description of
empirical reality, in so far as one takes it seriously in
a particular domain of applicability, the internal
view seems the more natural description.
โข Compare: position/momentum duality in QM. Equivalence of
frames in special relativity
28. Interpretation
โขThe internal point of view seems more natural for
theories of the whole world
โขEven if one views a theory as a partial description of
empirical reality, in so far as one takes it seriously in
a particular domain of applicability, the internal
view seems the more natural description.
โข Compare: position/momentum duality in QM. Equivalence of
frames in special relativity.
โข We should worry about the measurement problem, but it
is not necessarily part of what is here meant by โtheories
of the whole worldโ, because the statement is still true in
the classical limit, where we get Einstein gravity
29. โขButterfieldsโs puzzling scenario about truth (2014): Does
reality admit two or more complete descriptions which
โข (Different): are not notational variants of each other; and yet
โข (Success): are equally and wholly successful by all epistemic
criteria one should impose?
โขOn the external view, the two theories are not equally
successful because they describe different physical
quantities: only one of them may describe this world
โขOn the internal view, the two descriptions are equivalent
hence equally successful
โข If they turn out to be notational variants of each other (e.g.
different choices of gauge in a bigger theory) then the
philosophical conclusion is less exciting, but new physics is to
be expected. This is how dualities are often interpreted by
physicists: as providing heuristic guidance for theory
construction
โข If the two theories are not notational variants of each other,
then we do face the puzzling scenario!
30. โข On the external view, the two theories describe
different physics
โข The dual theory is only a tool that might be useful, but does
not describe the physics of our world
โข Here, the idea of โemergenceโ does not suggest itself
because whichever side describes our world, it does not
emerge from something else
โข On the internal view there is a one-to-one relation
between the values of physical quantities
โข Again emergence does not suggest itself: the two
descriptions are equivalent
โข If the duality is only approximate then there may be room
for emergence of space-time (analogy: thermodynamics
vs. statistical mechanics)
Emergence
32. โข The holographic relation may well be a bijective map
โข There is no reason in this case to think that one side is
more fundamental than the other (left-right)
โข But the thermodynamic limit introduces the emergence
of gravity in an uncontroversial sense (top-bottom)
Does Gravity Emerge?
33. At which level does this require holography?
โข The emergence of gravity only requires approximate holography
โข According to E. Verlinde, the microscopic bulk theory can be
dispensed with
34. Emergence of Space and Gravity
โข Gravity could thus emerge in the same way (via coarse
graining) in other situations where gauge/gravity duality
does not hold exactly (e.g. cosmological scenarios: dS/CFT)
โข But this idea can be applied more generally to AdS/CFT,
where the renormalization group flow introduces coarse
graining over high-energy degrees of freedom
โข In this case, Einstein gravity may emerge from the
fundamental bulk theory, whether the latter contains gravity
or not
35. Conclusions
โขIn holographic scenarios with an exact duality, the
microscopic surface theory is not necessarily more
fundamental than the microscopic bulk theory
โข The bulk does not emerge from the boundary in such
cases
โขHowever, the appearance of gravity in the
thermodynamic limit makes it a clear case of
emergence, connected with robustness and novelty
of behavior