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Holographic recipes for hot and dense strongly coupled matter SEWM-2008 Amsterdam Teniers the Younger (1610-1690) “The Alchemist”

Holographic recipes for hot and dense strongly coupled matter SEWM-2008 Amsterdam David Teniers the Younger (1610-1690) The Alchemist

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Page 1: Holographic recipes for hot and dense strongly coupled matter SEWM-2008 Amsterdam David Teniers the Younger (1610-1690) The Alchemist

Holographic recipes for hot and dense strongly coupled matter

SEWM-2008 Amsterdam

David Teniers the Younger (1610-1690) “The Alchemist”

Page 2: Holographic recipes for hot and dense strongly coupled matter SEWM-2008 Amsterdam David Teniers the Younger (1610-1690) The Alchemist

Andrei StarinetsUniversity of Southampton

Page 3: Holographic recipes for hot and dense strongly coupled matter SEWM-2008 Amsterdam David Teniers the Younger (1610-1690) The Alchemist

Outline

Introductory review of gauge/string duality

Finite temperature, holography and black hole physics

From gauge/string to gauge/gravity duality

Transport in strongly coupled gauge theories from black hole physics

First- and second-order hydrodynamics and dual gravity

Photon/dilepton emission rates from dual gravity

Other approaches

Quantum liquids and holography

Page 4: Holographic recipes for hot and dense strongly coupled matter SEWM-2008 Amsterdam David Teniers the Younger (1610-1690) The Alchemist

Over the last several years, holographic (gauge/gravity duality) methodswere used to study strongly coupled gauge theories at finite temperatureand density

These studies were motivated by the heavy-ion collision programs at RHICand LHC (ALICE detector) and the necessity to understand hot and densenuclear matter in the regime of intermediate coupling

As a result, we now have a better understanding of thermodynamicsand especially kinetics (transport) of strongly coupled gauge theories

Of course, these calculations are done for theoretical models such asN=4 SYM and its cousins (including non-conformal theories etc).

We don’t know for QCD

Page 5: Holographic recipes for hot and dense strongly coupled matter SEWM-2008 Amsterdam David Teniers the Younger (1610-1690) The Alchemist

What is string theory?

Page 6: Holographic recipes for hot and dense strongly coupled matter SEWM-2008 Amsterdam David Teniers the Younger (1610-1690) The Alchemist

Equations such as

describe the low energy limit of string theory

As long as the dilaton is small, and thus the string interactions are suppressed,this limit corresponds to classical 10-dim Einstein gravity coupled to certainmatter fields such as Maxwell field, p-forms, dilaton, fermions

Validity conditions for the classical (super)gravity approximation

- curvature invariants should be small:

- quantum loop effects (string interactions = dilaton) should be small:

In AdS/CFT duality, these two conditions translate into

and

Page 7: Holographic recipes for hot and dense strongly coupled matter SEWM-2008 Amsterdam David Teniers the Younger (1610-1690) The Alchemist

From brane dynamics to AdS/CFT correspondence

Open strings picture: dynamics of coincident D3 branes at low energy is described by

Closed strings picture: dynamics of coincident D3 branes at low energy is described by

conjecturedexact equivalence

Maldacena (1997); Gubser, Klebanov, Polyakov (1998); Witten (1998)

Page 8: Holographic recipes for hot and dense strongly coupled matter SEWM-2008 Amsterdam David Teniers the Younger (1610-1690) The Alchemist

AdS/CFT correspondence

conjecturedexact equivalence

Generating functional for correlation functions of gauge-invariant operators String partition function

In particular

Classical gravity action serves as a generating functional for the gauge theory correlators

Page 9: Holographic recipes for hot and dense strongly coupled matter SEWM-2008 Amsterdam David Teniers the Younger (1610-1690) The Alchemist

4D boundary

z

0

The bulk and the boundary in AdS/CFT correspondence

5D bulk (+5 internal dimensions)

UV/IR: the AdS metric is invariant under

z plays a role of inverse energy scale in 4D theory

Page 10: Holographic recipes for hot and dense strongly coupled matter SEWM-2008 Amsterdam David Teniers the Younger (1610-1690) The Alchemist

AdS/CFT correspondence: the role of J

satisfies linearized supergravity e.o.m. with b.c.

For a given operator , identify the source field , e.g.

To compute correlators of , one needs to solve the bulksupergravity e.o.m. for and compute the on-shell actionas a functional of the b.c.

Then, taking functional derivatives of gives

The recipe:

Warning: e.o.m. for different bulk fields may be coupled: need self-consistent solution

Page 11: Holographic recipes for hot and dense strongly coupled matter SEWM-2008 Amsterdam David Teniers the Younger (1610-1690) The Alchemist

supersymmetric Yang-Mills is the harmonic oscillator of the XXI century!

Page 12: Holographic recipes for hot and dense strongly coupled matter SEWM-2008 Amsterdam David Teniers the Younger (1610-1690) The Alchemist

• Field content:

• Action:

Gliozzi,Scherk,Olive’77

Brink,Schwarz,Scherk’77

(super)conformal field theory = coupling doesn’t run

supersymmetric YM theory

Page 13: Holographic recipes for hot and dense strongly coupled matter SEWM-2008 Amsterdam David Teniers the Younger (1610-1690) The Alchemist

AdS/CFT correspondence is the simplest example of the gauge/string (gauge/gravity) duality

Page 14: Holographic recipes for hot and dense strongly coupled matter SEWM-2008 Amsterdam David Teniers the Younger (1610-1690) The Alchemist

coupling

energy

Gauge/gravity duality and QCD

Page 15: Holographic recipes for hot and dense strongly coupled matter SEWM-2008 Amsterdam David Teniers the Younger (1610-1690) The Alchemist

coupling

energy

Gauge/gravity duality and QCD

Page 16: Holographic recipes for hot and dense strongly coupled matter SEWM-2008 Amsterdam David Teniers the Younger (1610-1690) The Alchemist

coupling

energy

Gauge/gravity duality and QCD

Page 17: Holographic recipes for hot and dense strongly coupled matter SEWM-2008 Amsterdam David Teniers the Younger (1610-1690) The Alchemist

Holography at finite temperature and density

Nonzero expectation values of energy and charge density translate intonontrivial background values of the metric (above extremality)=horizonand electric potential = CHARGED BLACK HOLE (with flat horizon)

temperature of the dual gauge theory

chemical potential of the dual theory

Page 18: Holographic recipes for hot and dense strongly coupled matter SEWM-2008 Amsterdam David Teniers the Younger (1610-1690) The Alchemist

Hydrodynamic properties of strongly interacting hot plasmas in 4 dimensions

can be related (for certain models!)

to fluctuations and dynamics of 5-dimensional black holes

Page 19: Holographic recipes for hot and dense strongly coupled matter SEWM-2008 Amsterdam David Teniers the Younger (1610-1690) The Alchemist

M,J,Q

Holographically dual system in thermal equilibrium

M, J, Q

T S

Gravitational fluctuations Deviations from equilibrium

????

and B.C.

Quasinormal spectrum

10-dim gravity4-dim gauge theory – large N,

strong coupling

+ fluctuations of other fields

Page 20: Holographic recipes for hot and dense strongly coupled matter SEWM-2008 Amsterdam David Teniers the Younger (1610-1690) The Alchemist

Computing transport coefficients from dual gravity

Assuming validity of the gauge/gravity duality, all transport coefficients are completely determined

by the lowest frequenciesin quasinormal spectra of the dual gravitational background

This determines kinetics in the regime of a thermal theorywhere the dual gravity description is applicable

(D.Son, A.S., hep-th/0205051, P.Kovtun, A.S., hep-th/0506184)

Transport coefficients and quasiparticle spectra can also beobtained from thermal spectral functions

Page 21: Holographic recipes for hot and dense strongly coupled matter SEWM-2008 Amsterdam David Teniers the Younger (1610-1690) The Alchemist

Computing transport coefficients from “first principles”

Kubo formulae allows one to calculate transport coefficients from microscopic models

In the regime described by a gravity dual the correlator can be computed using the gauge theory/gravity duality

Fluctuation-dissipation theory(Callen, Welton, Green, Kubo)

Page 22: Holographic recipes for hot and dense strongly coupled matter SEWM-2008 Amsterdam David Teniers the Younger (1610-1690) The Alchemist

First-order transport (kinetic) coefficients

* Expect Einstein relations such as to hold

Shear viscosity

Bulk viscosity

Charge diffusion constant

Supercharge diffusion constant

Thermal conductivity

Electrical conductivity

Page 23: Holographic recipes for hot and dense strongly coupled matter SEWM-2008 Amsterdam David Teniers the Younger (1610-1690) The Alchemist

First-order transport coefficients in N = 4 SYM in the limit

Shear viscosity

Bulk viscosity

Charge diffusion constant

Supercharge diffusion constant

Thermal conductivity

Electrical conductivity

(G.Policastro, 2008)

for non-conformal theories see Buchel et al; G.D.Moore et al Gubser et al.

Page 24: Holographic recipes for hot and dense strongly coupled matter SEWM-2008 Amsterdam David Teniers the Younger (1610-1690) The Alchemist

Electrical conductivity in SYM

Weak coupling:

Strong coupling:

* Charge susceptibility can be computed independently:

Einstein relation holds:

D.T.Son, A.S., hep-th/0601157

Page 25: Holographic recipes for hot and dense strongly coupled matter SEWM-2008 Amsterdam David Teniers the Younger (1610-1690) The Alchemist

Shear viscosity in SYM

Correction to : Buchel, Liu, A.S., hep-th/0406264

perturbative thermal gauge theoryS.Huot,S.Jeon,G.Moore, hep-ph/0608062

Buchel, 0805.2683 [hep-th]; Myers, Paulos, Sinha, 0806.2156 [hep-th]

Page 26: Holographic recipes for hot and dense strongly coupled matter SEWM-2008 Amsterdam David Teniers the Younger (1610-1690) The Alchemist

A viscosity bound conjecture

P.Kovtun, D.Son, A.S., hep-th/0309213, hep-th/0405231

Minimum of in units of

?? ??

Page 27: Holographic recipes for hot and dense strongly coupled matter SEWM-2008 Amsterdam David Teniers the Younger (1610-1690) The Alchemist

Is the bound dead? Y.Kats and P.Petrov, 0712.0743 [hep-th] “Effect of curvature squared corrections in AdS on the viscosity of the dual gauge theory”

superconformal Sp(N) gauge theory in d=4

M.~Brigante, H.~Liu, R.~C.~Myers, S.~Shenker and S.~Yaida, ``The Viscosity Bound and Causality Violation,'' 0802.3318 [hep-th], ``Viscosity Bound Violation in Higher Derivative Gravity,'' 0712.0805 [hep-th].

The “species problem” T.Cohen, hep-th/0702136, A.Dobado, F.Llanes-Estrada, hep-th/0703132

But see A.Buchel, 0804.3161 [hep-th]

Page 28: Holographic recipes for hot and dense strongly coupled matter SEWM-2008 Amsterdam David Teniers the Younger (1610-1690) The Alchemist

Second-order transport coefficients in N = 4 SYM in the limit

Relaxation time

Here we also used results from: S.Bhattacharyya,V.Hubeny,S.Minwalla,M.Rangamani, 0712.2456 [hep-th]

Generalized to CFT in D dim: Haack & Yarom, 0806.4602 [hep-th];

Finite ‘t Hooft coupling correction computed: Buchel and Paulos, 0806.0788 [hep-th]

Question: does this affect RHIC numerics?

Luzum and Romatschke, 0804.4015 [nuc-th]

Page 29: Holographic recipes for hot and dense strongly coupled matter SEWM-2008 Amsterdam David Teniers the Younger (1610-1690) The Alchemist

Hydrodynamics: fundamental d.o.f. = densities of conserved charges

Need to add constitutive relations!

Example: charge diffusion

[Fick’s law (1855)]

Conservation law

Constitutive relation

Diffusion equation

Dispersion relation

Expansion parameters:

Page 30: Holographic recipes for hot and dense strongly coupled matter SEWM-2008 Amsterdam David Teniers the Younger (1610-1690) The Alchemist

Viscosity/entropy ratio in QCD: current status

QCD: RHIC elliptic flow analysis suggests

Theories with gravity duals in the regimewhere the dual gravity description is valid

(universal limit)

QCD: (Indirect) LQCD simulations

H.Meyer, 0805.4567 [hep-th]

Trapped strongly correlated cold alkali atoms

Liquid Helium-3

T.Schafer, 0808.0734 [nucl-th]

Kovtun, Son & A.S; Buchel; Buchel & Liu, A.S

Page 31: Holographic recipes for hot and dense strongly coupled matter SEWM-2008 Amsterdam David Teniers the Younger (1610-1690) The Alchemist

Chernai, Kapusta, McLerran, nucl-th/0604032

Page 32: Holographic recipes for hot and dense strongly coupled matter SEWM-2008 Amsterdam David Teniers the Younger (1610-1690) The Alchemist

Supersymmetric sound mode (“phonino”) in

Conserved charge

Hydrodynamic mode (infinitely slowly relaxing fluctuation of the charge density)

Hydro polein the retardedcorrelator of thecharge density

Sound wave pole:

Supersound wave pole:

Lebedev & Smilga, 1988 (see also Kovtun & Yaffe, 2003)

Page 33: Holographic recipes for hot and dense strongly coupled matter SEWM-2008 Amsterdam David Teniers the Younger (1610-1690) The Alchemist

Sound and supersymmetric sound in

Sound mode:

Supersound mode:

In 4d CFT

Quasinormal modes in dual gravity

Graviton:

Gravitino:

Page 34: Holographic recipes for hot and dense strongly coupled matter SEWM-2008 Amsterdam David Teniers the Younger (1610-1690) The Alchemist

Photon and dilepton emission from supersymmetric Yang-Mills plasmaS. Caron-Huot, P. Kovtun, G. Moore, A.S., L.G. Yaffe, hep-th/0607237

Page 35: Holographic recipes for hot and dense strongly coupled matter SEWM-2008 Amsterdam David Teniers the Younger (1610-1690) The Alchemist

Photoproduction rate in SYM

(Normalized) photon production rate in SYM for various values of ‘t Hooft coupling

Page 36: Holographic recipes for hot and dense strongly coupled matter SEWM-2008 Amsterdam David Teniers the Younger (1610-1690) The Alchemist

Now consider strongly interacting systems at finite density and LOW temperature

Page 37: Holographic recipes for hot and dense strongly coupled matter SEWM-2008 Amsterdam David Teniers the Younger (1610-1690) The Alchemist

“Holographic recipes at finite density and low temperature”

This part of the talk -

- is based on the paper

“Zero Sound from Holography”

arXiv: 0806.3796 [hep-th]

Andreas Karch Dam Thanh Son

by

A.S.

Page 38: Holographic recipes for hot and dense strongly coupled matter SEWM-2008 Amsterdam David Teniers the Younger (1610-1690) The Alchemist

Probing quantum liquids with holography

Quantum liquid in p+1 dim

Low-energy elementary excitations

Specific heat at low T

Quantum Bose liquid

Quantum Fermi liquid (Landau FLT)

phonons

fermionic quasiparticles +bosonic branch (zero sound)

Departures from normal Fermi liquid occur in

- 3+1 and 2+1 –dimensional systems with strongly correlated electrons

- In 1+1 –dimensional systems for any strength of interaction (Luttinger liquid)

One can apply holography to study strongly coupled Fermi systems at low T

Page 39: Holographic recipes for hot and dense strongly coupled matter SEWM-2008 Amsterdam David Teniers the Younger (1610-1690) The Alchemist

L.D.Landau (1908-1968)

Page 40: Holographic recipes for hot and dense strongly coupled matter SEWM-2008 Amsterdam David Teniers the Younger (1610-1690) The Alchemist

The simplest candidate with a known holographic description is

at finite temperature T and nonzero chemical potential associated with the“baryon number” density of the charge

There are two dimensionless parameters:

is the baryon number density is the hypermultiplet mass

The holographic dual description in the limit is given by the D3/D7 system, with D3 branes replaced by the AdS-Schwarzschild geometry and D7 branes embedded in it as probes.

Karch & Katz, hep-th/0205236

Page 41: Holographic recipes for hot and dense strongly coupled matter SEWM-2008 Amsterdam David Teniers the Younger (1610-1690) The Alchemist

AdS-Schwarzschild black hole (brane) background

D7 probe branes

The worldvolume U(1) field couples to the flavor current at the boundary

Nontrivial background value of corresponds to nontrivial expectation value of

We would like to compute

- the specific heat at low temperature

- the charge density correlator

Page 42: Holographic recipes for hot and dense strongly coupled matter SEWM-2008 Amsterdam David Teniers the Younger (1610-1690) The Alchemist

The specific heat (in p+1 dimensions):

(note the difference with Fermi and Bose systems)

The (retarded) charge density correlator has a pole corresponding to a propagating mode (zero sound) - even at zero temperature

(note that this is NOT a superfluid phonon whose attenuation scales as )

New type of quantum liquid?

Page 43: Holographic recipes for hot and dense strongly coupled matter SEWM-2008 Amsterdam David Teniers the Younger (1610-1690) The Alchemist

Other avenues of (related) research

Bulk viscosity for non-conformal theories (Buchel, Gubser,…)

Non-relativistic gravity duals (Son, McGreevy,… )

Gravity duals of theories with SSB (Kovtun, Herzog,…)

Bulk from the boundary (Janik,…)

Navier-Stokes equations and their generalization from gravity (Minwalla,…)

Quarks moving through plasma (Chesler, Yaffe, Gubser,…)

Page 44: Holographic recipes for hot and dense strongly coupled matter SEWM-2008 Amsterdam David Teniers the Younger (1610-1690) The Alchemist
Page 45: Holographic recipes for hot and dense strongly coupled matter SEWM-2008 Amsterdam David Teniers the Younger (1610-1690) The Alchemist

THANK YOU

Page 46: Holographic recipes for hot and dense strongly coupled matter SEWM-2008 Amsterdam David Teniers the Younger (1610-1690) The Alchemist

Figure: an artistic impression from Myers and Vazquez, 0804.2423 [hep-th]

Energy density vs temperature for various gauge theories

Ideal gasof quarksand gluons

Ideal gasof hadrons

Page 47: Holographic recipes for hot and dense strongly coupled matter SEWM-2008 Amsterdam David Teniers the Younger (1610-1690) The Alchemist

Conclusions

The program of computing first- and second-order transport coefficients in N=4 SYM at strong coupling and large number of colors is essentially complete

These calculations are helpful in numerical simulations of non-equilibrium QCD and stimulated developments in other fields such as LQCD, pQCD, condmat

LHC (ALICE) will provide more data at higher T

Need better understanding of

- thermalization, isotropisation, and time evolution [Janik et al.]

- corrections from higher-derivative terms [Kats & Petrov; Brigante,Myers,Shenker,Yaida]

[ Buchel, Myers, Paulos, Sinha, 0808.1837 [hep-th] ]

At low temperature and finite density, does holography identify a new type of quantum liquid?

(perturbative study of SUSY models at finite temperature and density would be very helpful)

Page 48: Holographic recipes for hot and dense strongly coupled matter SEWM-2008 Amsterdam David Teniers the Younger (1610-1690) The Alchemist

Luzum and Romatschke, 0804.4015 [nuc-th]

Elliptic flow with Glauber initial conditions

Page 49: Holographic recipes for hot and dense strongly coupled matter SEWM-2008 Amsterdam David Teniers the Younger (1610-1690) The Alchemist

Luzum and Romatschke, 0804.4015 [nuc-th]

Elliptic flow with color glass condensate initial conditions

Page 50: Holographic recipes for hot and dense strongly coupled matter SEWM-2008 Amsterdam David Teniers the Younger (1610-1690) The Alchemist

Is the bound dead? Y.Kats and P.Petrov, 0712.0743 [hep-th] “Effect of curvature squared corrections in AdS on the viscosity of the dual gauge theory”

superconformal Sp(N) gauge theory in d=4

M.~Brigante, H.~Liu, R.~C.~Myers, S.~Shenker and S.~Yaida, ``The Viscosity Bound and Causality Violation,'' 0802.3318 [hep-th], ``Viscosity Bound Violation in Higher Derivative Gravity,'' 0712.0805 [hep-th].

The “species problem” T.Cohen, hep-th/0702136, A.Dobado, F.Llanes-Estrada, hep-th/0703132

But see A.Buchel, 0804.3161 [hep-th]

Page 51: Holographic recipes for hot and dense strongly coupled matter SEWM-2008 Amsterdam David Teniers the Younger (1610-1690) The Alchemist

Hydrodynamics is an effective theory, valid for sufficiently small momenta

First-order hydro eqs are parabolic. They imply instant propagation of signals.

Second-order hydrodynamics

This is not a conceptual problem since hydrodynamics becomes “acausal” onlyoutside of its validity range but it is very inconvenient for numerical work onNavier-Stokes equations where it leads to instabilities [Hiscock & Lindblom, 1985]

These problems are resolved by considering next order in derivative expansion,i.e. by adding to the hydro constitutive relations all possible second-order termscompatible with symmetries (e.g. conformal symmetry for conformal plasmas)

Page 52: Holographic recipes for hot and dense strongly coupled matter SEWM-2008 Amsterdam David Teniers the Younger (1610-1690) The Alchemist

Andrei StarinetsUniversity of Southampton

Page 53: Holographic recipes for hot and dense strongly coupled matter SEWM-2008 Amsterdam David Teniers the Younger (1610-1690) The Alchemist

Second-order hydrodynamics in

Here we also used results from: S.Bhattacharyya,V.Hubeny,S.Minwalla,M.Rangamani, 0712.2456 [hep-th]

Second-order conformal hydrodynamics can be systematically constructed

Using AdS/CFT, all new transport coefficients for N=4 SYM can be computed

Question: does this affect RHIC numerics?

Generalized to CFT in D dim: Haack & Yarom, 0806.4602 [hep-th];

Finite ‘t Hooft coupling correction computed: Buchel and Paulos, 0806.0788 [hep-th]

Page 54: Holographic recipes for hot and dense strongly coupled matter SEWM-2008 Amsterdam David Teniers the Younger (1610-1690) The Alchemist

Second-order conformal hydrodynamics

Page 55: Holographic recipes for hot and dense strongly coupled matter SEWM-2008 Amsterdam David Teniers the Younger (1610-1690) The Alchemist

Hydrodynamic d.o.f. = densities of conserved charges

or

(4 d.o.f.)(4 equations)

Derivative expansion in hydrodynamics: first order

Page 56: Holographic recipes for hot and dense strongly coupled matter SEWM-2008 Amsterdam David Teniers the Younger (1610-1690) The Alchemist

Supersymmetric sound mode (“phonino”) in

Conserved charge

Hydrodynamic mode (infinitely slowly relaxing fluctuation of the charge density)

Hydro polein the retardedcorrelator of thecharge density

Sound wave pole:

Supersound wave pole:

Lebedev & Smilga, 1988 (see also Kovtun & Yaffe, 2003)

Page 57: Holographic recipes for hot and dense strongly coupled matter SEWM-2008 Amsterdam David Teniers the Younger (1610-1690) The Alchemist

Sound and supersymmetric sound in

Sound mode:

Supersound mode:

In 4d CFT

Quasinormal modes in dual gravity

Graviton:

Gravitino:

Page 58: Holographic recipes for hot and dense strongly coupled matter SEWM-2008 Amsterdam David Teniers the Younger (1610-1690) The Alchemist

Second-order conformal hydrodynamics

Page 59: Holographic recipes for hot and dense strongly coupled matter SEWM-2008 Amsterdam David Teniers the Younger (1610-1690) The Alchemist

Second-order Israel-Stewart conformal hydrodynamics

Israel-Stewart

Page 60: Holographic recipes for hot and dense strongly coupled matter SEWM-2008 Amsterdam David Teniers the Younger (1610-1690) The Alchemist

First-order conformal hydrodynamics

Weyl transformations:

In first-order hydro this implies:

Thus, in first-order hydro:

Page 61: Holographic recipes for hot and dense strongly coupled matter SEWM-2008 Amsterdam David Teniers the Younger (1610-1690) The Alchemist

Still, acausality is unpleasant, especially for numerical simulations, where it leads to instabilities

It would be convenient to have a UV completion (at strong and weak coupling)

Israel-Stewart theory is such a completion built with e.g. Boltzmann eq

AdS/CFT shows that at strong coupling, I-S theory is incomplete

Page 62: Holographic recipes for hot and dense strongly coupled matter SEWM-2008 Amsterdam David Teniers the Younger (1610-1690) The Alchemist

AdS/CFT correspondence

Yang-Mills theory with

N=4 supersymmetry

String theory on

AdS5xS5 background

Maldacena’97

Gubser,Klebanov,Polyakov’98

Witten’98Exact equivalence

Page 63: Holographic recipes for hot and dense strongly coupled matter SEWM-2008 Amsterdam David Teniers the Younger (1610-1690) The Alchemist

A viscosity bound conjecture

P.Kovtun, D.Son, A.S., hep-th/0309213, hep-th/0405231

Minimum of in units of

?? ??

Page 64: Holographic recipes for hot and dense strongly coupled matter SEWM-2008 Amsterdam David Teniers the Younger (1610-1690) The Alchemist

A hand-waving argument

Gravity duals fix the coefficient:

Thus ?

Page 65: Holographic recipes for hot and dense strongly coupled matter SEWM-2008 Amsterdam David Teniers the Younger (1610-1690) The Alchemist

The “species problem”

A.Dobado, F.Llanes-Estrada, hep-th/0703132

T.Cohen, hep-th/0702136

Buckminsterfullerene

a.k.a.”buckyball”

Classical dilute gas with a LARGE number of components

has a large Gibbs mixing entropy

To have with

need (Dam Son, 2007)

To have need

species

Page 66: Holographic recipes for hot and dense strongly coupled matter SEWM-2008 Amsterdam David Teniers the Younger (1610-1690) The Alchemist

Can we test

experimentally?

Heavy ion collisions - experiments at RHIC

(Indirect) lattice QCD simulations

Trapped atoms – strongly interacting Fermi systems

A characteristic feature of systems saturating the bound: strong interactions

Page 67: Holographic recipes for hot and dense strongly coupled matter SEWM-2008 Amsterdam David Teniers the Younger (1610-1690) The Alchemist

QCD kinetics

Viscosity is ONE of the parameters used in the hydro modelsdescribing the azimuthal anisotropy of particle distribution at RHIC

-elliptic flow forparticle species “i”

Elliptic flow reproduced for

e.g. Baier, Romatschke, nucl-th/0610108

Perturbative QCD:

SYM:

Chernai, Kapusta, McLerran, nucl-th/0604032

Page 68: Holographic recipes for hot and dense strongly coupled matter SEWM-2008 Amsterdam David Teniers the Younger (1610-1690) The Alchemist

Elliptic flow from relativistic hydro simulations

H.Song and U.Heinz, 0712.3715 [nucl-th]

(Israel-Stewart formalism)

Page 69: Holographic recipes for hot and dense strongly coupled matter SEWM-2008 Amsterdam David Teniers the Younger (1610-1690) The Alchemist

Experimental and theoretical motivation

Heavy ion collision program at RHIC, LHC (2000-2008-2020 ??)

Studies of hot and dense nuclear matter

Abundance of experimental results, poor theoretical understanding:

- the collision apparently creates a fireball of “quark-gluon fluid”

- need to understand both thermodynamics and kinetics

-in particular, need theoretical predictions for parameters entering equations of relativistic hydrodynamics – viscosity etc –

computed from the underlying microscopic theory (thermal QCD)

-this is difficult since the fireball is a strongly interacting nuclear fluid,not a dilute gas

Page 70: Holographic recipes for hot and dense strongly coupled matter SEWM-2008 Amsterdam David Teniers the Younger (1610-1690) The Alchemist

Predictions of the second-order conformal hydrodynamics

Sound dispersion:

Kubo:

Page 71: Holographic recipes for hot and dense strongly coupled matter SEWM-2008 Amsterdam David Teniers the Younger (1610-1690) The Alchemist

New transport coefficients in

Sound dispersion:

Kubo:

SYM

Page 72: Holographic recipes for hot and dense strongly coupled matter SEWM-2008 Amsterdam David Teniers the Younger (1610-1690) The Alchemist

Sound dispersion in

analytic approximation

analytic approximation

Page 73: Holographic recipes for hot and dense strongly coupled matter SEWM-2008 Amsterdam David Teniers the Younger (1610-1690) The Alchemist

Luzum and Romatschke, 0804.4015 [nuc-th]

The effect of the second-order coefficients

Page 74: Holographic recipes for hot and dense strongly coupled matter SEWM-2008 Amsterdam David Teniers the Younger (1610-1690) The Alchemist

Spectral function and quasiparticles in finite-temperature “AdS + IR cutoff”

model

Page 75: Holographic recipes for hot and dense strongly coupled matter SEWM-2008 Amsterdam David Teniers the Younger (1610-1690) The Alchemist

Computing transport coefficients from dual gravity – various methods

1. Green-Kubo formulas (+ retarded correlator from gravity)

2. Poles of the retarded correlators

3. Lowest quasinormal frequency of the dual background

4. The membrane paradigm

Page 76: Holographic recipes for hot and dense strongly coupled matter SEWM-2008 Amsterdam David Teniers the Younger (1610-1690) The Alchemist

Holographic models with fundamental fermions

Additional parameter makes life more interesting…

Thermal spectral functionsof flavor currents

R.Myers, A.S., R.Thomson, 0706.0162 [hep-th]

Page 77: Holographic recipes for hot and dense strongly coupled matter SEWM-2008 Amsterdam David Teniers the Younger (1610-1690) The Alchemist

Example: stress-energy tensor correlator in

in the limit

Finite temperature, Mink:

Zero temperature, Euclid:

(in the limit )

The pole (or the lowest quasinormal freq.)

Compare with hydro:

In CFT:

Also, (Gubser, Klebanov, Peet, 1996)

Page 78: Holographic recipes for hot and dense strongly coupled matter SEWM-2008 Amsterdam David Teniers the Younger (1610-1690) The Alchemist

Example 2 (continued): stress-energy tensor correlator in

in the limit

Finite temperature, Mink:

Zero temperature, Euclid:

(in the limit )

The pole (or the lowest quasinormal freq.)

Compare with hydro:

Page 79: Holographic recipes for hot and dense strongly coupled matter SEWM-2008 Amsterdam David Teniers the Younger (1610-1690) The Alchemist

Viscosity-entropy ratio of a trapped Fermi gas

T.Schafer, cond-mat/0701251

(based on experimental results by Duke U. group, J.E.Thomas et al., 2005-06)

Page 80: Holographic recipes for hot and dense strongly coupled matter SEWM-2008 Amsterdam David Teniers the Younger (1610-1690) The Alchemist

Chernai, Kapusta, McLerran, nucl-th/0604032

Page 81: Holographic recipes for hot and dense strongly coupled matter SEWM-2008 Amsterdam David Teniers the Younger (1610-1690) The Alchemist

Viscosity “measurements” at RHIC

Viscosity is ONE of the parameters used in the hydro modelsdescribing the azimuthal anisotropy of particle distribution

-elliptic flow forparticle species “i”

Elliptic flow reproduced for

Is it so? Heinz and Song, 2007

Perturbative QCD:

SYM:

Chernai, Kapusta, McLerran, nucl-th/0604032

Page 82: Holographic recipes for hot and dense strongly coupled matter SEWM-2008 Amsterdam David Teniers the Younger (1610-1690) The Alchemist

Two-point correlation function of

stress-energy tensor Field theory

Zero temperature:

Finite temperature:

Dual gravity

Five gauge-invariant combinations of and other fields determine

obey a system of coupled ODEs Their (quasinormal) spectrum determines singularities of the correlator

Page 83: Holographic recipes for hot and dense strongly coupled matter SEWM-2008 Amsterdam David Teniers the Younger (1610-1690) The Alchemist

Computing finite-temperature correlation functions from gravity

Need to solve 5d e.o.m. of the dual fields propagating in asymptotically AdS space

Can compute Minkowski-space 4d correlators

Gravity maps into real-time finite-temperature formalism (Son and A.S., 2001; Herzog and Son, 2002)

Page 84: Holographic recipes for hot and dense strongly coupled matter SEWM-2008 Amsterdam David Teniers the Younger (1610-1690) The Alchemist

Outlook

Gravity dual description of thermalization ?

Beyond hydrodynamics: AdS/CFT vs Israel-StewartBaier, Romatschke, Stephanov, Son, A.S., to appear

Understanding 1/N corrections

Phonino

The role of membrane paradigme?

Page 85: Holographic recipes for hot and dense strongly coupled matter SEWM-2008 Amsterdam David Teniers the Younger (1610-1690) The Alchemist

M,J,Q

Holographically dual system in thermal equilibrium

M, J, Q

T S

Gravitational fluctuations Deviations from equilibrium

????

and B.C.

Quasinormal spectrum

10-dim gravity4-dim gauge theory – large N,

strong coupling

+ fluctuations of other fields

Page 86: Holographic recipes for hot and dense strongly coupled matter SEWM-2008 Amsterdam David Teniers the Younger (1610-1690) The Alchemist

Chernai, Kapusta, McLerran, nucl-th/0604032

QCD

Page 87: Holographic recipes for hot and dense strongly coupled matter SEWM-2008 Amsterdam David Teniers the Younger (1610-1690) The Alchemist

Now look at the correlators obtained from gravity

The correlator has poles at

The speed of sound coincides with the hydro prediction!

Page 88: Holographic recipes for hot and dense strongly coupled matter SEWM-2008 Amsterdam David Teniers the Younger (1610-1690) The Alchemist

Similarly, one can analyze another conserved quantity – energy-momentum tensor:

This is equivalent to analyzing fluctuations of energy and pressure

We obtain a dispersion relation for the sound wave:

Page 89: Holographic recipes for hot and dense strongly coupled matter SEWM-2008 Amsterdam David Teniers the Younger (1610-1690) The Alchemist

Universality of

Theorem:

For a thermal gauge theory, the ratio of shear viscosity to entropy density is equal to in the regime described by a dual gravity theory

Remarks:

• Extended to non-zero chemical potential:

• Extended to models with fundamental fermions in the limit

• String/Gravity dual to QCD is currently unknown

Benincasa, Buchel, Naryshkin, hep-th/0610145

Mateos, Myers, Thomson, hep-th/0610184

Page 90: Holographic recipes for hot and dense strongly coupled matter SEWM-2008 Amsterdam David Teniers the Younger (1610-1690) The Alchemist

Three roads to universality of

The absorption argument D. Son, P. Kovtun, A.S., hep-th/0405231

Direct computation of the correlator in Kubo formula from AdS/CFT A.Buchel, hep-th/0408095

“Membrane paradigm” general formula for diffusion coefficient + interpretation as lowest quasinormal frequency = pole of the shear mode correlator + Buchel-Liu theorem

P. Kovtun, D.Son, A.S., hep-th/0309213, A.S., to appear, P.Kovtun, A.S., hep-th/0506184, A.Buchel, J.Liu, hep-th/0311175

Page 91: Holographic recipes for hot and dense strongly coupled matter SEWM-2008 Amsterdam David Teniers the Younger (1610-1690) The Alchemist

Universality of shear viscosity in the regime described by gravity duals

Graviton’s component obeys equation for a minimally coupled massless scalar. But then .

Since the entropy (density) is we get

Page 92: Holographic recipes for hot and dense strongly coupled matter SEWM-2008 Amsterdam David Teniers the Younger (1610-1690) The Alchemist

Chernai, Kapusta, McLerran, nucl-th/0604032

Page 93: Holographic recipes for hot and dense strongly coupled matter SEWM-2008 Amsterdam David Teniers the Younger (1610-1690) The Alchemist

Hydrodynamics predicts that the retarded correlator

has a “sound wave” pole at

Moreover, in conformal theory

Predictions of hydrodynamics

Page 94: Holographic recipes for hot and dense strongly coupled matter SEWM-2008 Amsterdam David Teniers the Younger (1610-1690) The Alchemist

QCD thermodynamics

QCD deconfinement transition (lattice data)

Energy densityvs

temperature

Page 95: Holographic recipes for hot and dense strongly coupled matter SEWM-2008 Amsterdam David Teniers the Younger (1610-1690) The Alchemist

Computing transport coefficients from “first principles”

Kubo formulae allows one to calculate transport coefficients from microscopic models

In the regime described by a gravity dual the correlator can be computed using the gauge theory/gravity duality

Fluctuation-dissipation theory(Callen, Welton, Green, Kubo)