Holograpic Transport Coeffients Equation of State and Viscosities *)

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B. Kampfer I Institute of Radiation Physics I www.hzdr.de Member of the Helmholtz Association page 1 B. Kampfer I Institute of Radiation Physics I www.hzdr.de Holograpic Transport Coeffients Equation of State and Viscosities *) (AdS/QCD) R. Yaresko, B. Kämpfer Helmholtz-Zentrum Dresden-Rossendorf and Technische Universität Dresden *) 1403.3581, 1306.0214

description

Holograpic Transport Coeffients Equation of State and Viscosities *) (AdS/QCD). R. Yaresko, B. Kämpfer. Helmholtz-Zentrum Dresden-Rossendorf and Technische Universität Dresden. *) 1403.3581, 1306.0214. from Mocsy, Sorensen - PowerPoint PPT Presentation

Transcript of Holograpic Transport Coeffients Equation of State and Viscosities *)

Page 1: Holograpic Transport Coeffients          Equation of State and Viscosities *)

B. Kampfer I Institute of Radiation Physics I www.hzdr.deMember of the Helmholtz Associationpage 1

B. Kampfer I Institute of Radiation Physics I www.hzdr.de

Holograpic Transport Coeffients Equation of State and Viscosities *) (AdS/QCD)

R. Yaresko, B. Kämpfer

Helmholtz-Zentrum Dresden-Rossendorf and Technische Universität Dresden

*) 1403.3581, 1306.0214

Page 2: Holograpic Transport Coeffients          Equation of State and Viscosities *)

B. Kampfer I Institute of Radiation Physics I www.hzdr.deMember of the Helmholtz Associationpage 2

Big Bang

Inflation CMB COBE, WMAP, Planck BICEP2

, PHENIX, ALICE…

fromMocsy, Sorensen1008.3381

HYDRO:EoS +viscosities

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B. Kampfer I Institute of Radiation Physics I www.hzdr.deMember of the Helmholtz Associationpage 3

water:

viscosity is importantfor flow pattern and splashes

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B. Kampfer I Institute of Radiation Physics I www.hzdr.deMember of the Helmholtz Associationpage 4

Bulk Viscosity Could Matter

Dusling, Schafer, PRC 85 (2012) 044909

pQCD (leading log):

48

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B. Kampfer I Institute of Radiation Physics I www.hzdr.deMember of the Helmholtz Associationpage 5

Bulk Viscosity Matters

Noronha-Hostler, Denicol, Noronha, Andrade, Grassi, Phys.Rev. C88 (2013) 044916

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B. Kampfer I Institute of Radiation Physics I www.hzdr.deMember of the Helmholtz Associationpage 6

Bulk Viscosity Can Matter

coupling of conformal anomaly to photons

Basar, Kharzeev, Skokov, PRL 109 (2012) 202303

solution of photon-v2 puzzle?

data: PHENIXPRL 109 (2012) 122302

Tuchin, arXiv:1301.0099

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B. Kampfer I Institute of Radiation Physics I www.hzdr.deMember of the Helmholtz Associationpage 7

orig.Huovinen, Int.J.Mod.Phys. E22 (2013) 1330029

bulk viscosity

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B. Kampfer I Institute of Radiation Physics I www.hzdr.deMember of the Helmholtz Associationpage 8

Bluhm et al., PLB 709 (2012) 77, PRC 84 (2011) 025201

Compilation of Lattice Results & QPM

(1) EoS

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a = 3.78, b = - 0.3

(2) relaxation time

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B. Kampfer I Institute of Radiation Physics I www.hzdr.deMember of the Helmholtz Associationpage 10

Holography

physics in D + N D

quantum gravity QFT

e.g. AdS/CFT: 1997:Maldacena,Gubser et al. Witten

isometries symmetry

classical gravity strongly coupled QFT`t Hooft coupling and Nc large

Page 11: Holograpic Transport Coeffients          Equation of State and Viscosities *)

B. Kampfer I Institute of Radiation Physics I www.hzdr.deMember of the Helmholtz Associationpage 11

boundary

blackness funct. (simple zero horizon)

r = const: Minkowski slicesr infty: boundary

: holographic coordinate (renorm.) scale Z 1/r

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B. Kampfer I Institute of Radiation Physics I www.hzdr.deMember of the Helmholtz Associationpage 12

gravity dual of QCD is unknown

recipe: breaking of conf. symmetry duality with non-conf. QFT

bottom-up appr.: mimicing thermal QCD features/expectations by 1 scalar („dilaton“) kinetic term + potential + by 1 gauge field

T

n

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B. Kampfer I Institute of Radiation Physics I www.hzdr.deMember of the Helmholtz Associationpage 13

gravity setup

metric ansatz (Riemann)

Einstein - Hilbert

gauged radial coordinate scale

Gubser et al. PRL 101 (2008) 131601, PRD 78 (2008) 086007

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B. Kampfer I Institute of Radiation Physics I www.hzdr.deMember of the Helmholtz Associationpage 14

U = V / (3 V‘)

EoS s(T)

0

AdSBekenstein

Hawking

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B. Kampfer I Institute of Radiation Physics I www.hzdr.deMember of the Helmholtz Associationpage 15

Kiritsis et al.: - 2 scalar eqs. for X‘, Y‘ - 2 quadratures LT, G_5 s

phi_H

UV IR

G_5

s

LTLTc

Kiritsis et al.:p(Tc) = 0

open questions: - a unique (master) V - V vs. phase transition

engineering the potential: EoS V

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B. Kampfer I Institute of Radiation Physics I www.hzdr.deMember of the Helmholtz Associationpage 16

bottom-up approach: EoS (lattice QCD) dilaton potential

ansatz: Gubser type pot. + polynom. distortions

T/Tc vs. TL:from T(s/T^3)min. or turning

G5: from s/T^3

exp. functs. from supergravity pots.

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B. Kampfer I Institute of Radiation Physics I www.hzdr.deMember of the Helmholtz Associationpage 17

lattice QCD, SU(3) gauge theory, Borsanyi et al., JHEP 1207 (2012) 056 consistent with Boyd et al., NPB 469 (1996) 419

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B. Kampfer I Institute of Radiation Physics I www.hzdr.deMember of the Helmholtz Associationpage 18

bulk viscosity

shear viscosity is independent of V

Gubser et al., JHEP 0808 (2008) 085

KSS, JHEP 0310 (2003) 064

Policastro, Son, Starinets, PRL 87 (2001) 081601

Eling, Oz, JHEP 1106 (2011) 007cf. Buchel et al., JHEP 1109 (2011) 095

0

AdS

= (d log s / d log phi_H)-2

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benefit: w/o further input spectral functions transport coefficients

as in QPM (Bluhm et al.)

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B. Kampfer I Institute of Radiation Physics I www.hzdr.deMember of the Helmholtz Associationpage 20

bulk viscosity is not universal (as, e.g. shear viscosity/entropy) sensitive dependence on pot. parameters

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B. Kampfer I Institute of Radiation Physics I www.hzdr.deMember of the Helmholtz Associationpage 21

Kiritsis et al. Model

Tc from p = 0, beta function, confinement

J. Knaute (2014)

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B. Kampfer I Institute of Radiation Physics I www.hzdr.deMember of the Helmholtz Associationpage 22

Is the Potential Unique?

10 Tc Tcboundary (UV)

nearly the same EoS & bulk viscosity

also for Kititsis pot. (boundary at phi infty)

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B. Kampfer I Institute of Radiation Physics I www.hzdr.deMember of the Helmholtz Associationpage 23

including quarks

WB Collab.Phys.Lett. B730 (2014) 99

A. Bazavov [hotQCD], talk at QM2014, Tuesday

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DeWolfe , Gubser, Rosen, Phys.Rev. D84 (2011) 126014, 83 (2011) 086005

two dilaton „potentials“:

models with CEP

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Summary

after precise adjustment of EoS at lattice data here: SU(3) YM

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B. Kampfer I Institute of Radiation Physics I www.hzdr.deMember of the Helmholtz Associationpage 26

Outlook

spectral functions & medium on equal footing beyond soft-wall models

temperature dependence of eta/s beyond Einstein-Hilbert action

mu > 0 CEP: DeWolfe, Gubser, Rosen, PRD 83 (2011) 086005, PRD 84 (2011) 126014

Cremonini, Gursoy, Szepietowski, JHEP 08 (2012) 167

and all the other transport coefficients

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B. Kampfer I Institute of Radiation Physics I www.hzdr.deMember of the Helmholtz Associationpage 27

AdS/QCD, soft-wall model, Cui. Takeuchi, Wu, 1112.5923

(T in GeV)

JHEP 1204 (2012) 144

meson in vector channel

Abelian field strength of Vsoft-wall model:

mass shift

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B. Kampfer I Institute of Radiation Physics I www.hzdr.deMember of the Helmholtz Associationpage 28

AdS/QCD, soft-wall model, Colangelo, Giannuzzi, Nicotri, 1201.1564, JHEP 1205 (2012) 076

Schwarzschild BH Reissner-Nordstrom BH: chem. pot.

vision: beyond soft-wall ansatz dilaton consistent with EoSproblem: missing unique QCD results with quarks

mass shift + broadening

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B. Kampfer I Institute of Radiation Physics I www.hzdr.deMember of the Helmholtz Associationpage 29

AdS/QCD

5D Riemann: x,z 4D Minkowski: x

semi-class. gravity strongly coupled gauge theo.

X(x, z) gauge-inv. Operators (x)

asymp. AdS black brane: T (Hawking) s (Bekenstein)

semi-class. functional correlation functions breaking conf. sym. by mass scale, e.g. dilation + potential

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AdS/CFT Emissivities

Baier,Stricker, Taanila, Vuorinen, Phys.Rev. D86 (2012) 081901, JHEP 1207 (2012) 094

at T > 200 MeV, one obtains the thermalization time scale ~ 0.1 fm/c, which one might compare with the typical production time of dileptons with mass/energy larger than 5 GeV, tau_p < 0.04 fm/c. It appears that dilepton pairs produced early on have a reasonable chance to escape the system while it is still out of thermal equilibrium.

problem of particle production in dynamical systems

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B. Kampfer I Institute of Radiation Physics I www.hzdr.deMember of the Helmholtz Associationpage 31

with lin. fluct.

quark-mesonmodel

mfa

F. Wunderlich

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B. Kampfer I Institute of Radiation Physics I www.hzdr.deMember of the Helmholtz Associationpage 32

lin. fluct.

50 MeVphotons

isentropes

lin. fluct.