Holographic Thermalization Irina Arefeva Steklov Mathematical Institute RAN

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Holographic Thermalization Irina Aref'eva Steklov Mathematical Institute, RAN, Moscow International Conference on Physics “In

Holographic Thermalization Irina Aref'eva Steklov Mathematical Institute, RAN, Moscow International Conference on Physics “In Search of Fundamental Symmetries” dedicated to the 90 -th birthday anniversary of Yuri Victorovich Novozhilov

Yuri Victorovich Novozhilov

Yuri Victorovich Novozhilov

Yuri Victorovich Novozhilov

Yuri Victorovich Novozhilov

Hologhraphic thermalization Thermalization of QFT in Minkowski D-dim spacetime Black Hole formation in Anti

Hologhraphic thermalization Thermalization of QFT in Minkowski D-dim spacetime Black Hole formation in Anti de Sitter (D+1)-dim space-time

Models of BH creation in D=5 and their relations with HIC in D=4 perturbation.

Models of BH creation in D=5 and their relations with HIC in D=4 perturbation. S of Ad. S • Ad. S/CFT correspondence 4 -dim of colliding matter Main idea: make some perturbation. S of Ad. S metric that near the boundary “mimic” the mater (heavy ions) collisions and see what happens.

Hologhraphic thermalization How to “mimic” the heavy ions collision Models: 1) shock waves collision

Hologhraphic thermalization How to “mimic” the heavy ions collision Models: 1) shock waves collision in Ad. S 2) infalling shell

Hologhraphic thermalization Physical quantities that we expect to get: D=5 Ad. S D=4 Minkowski

Hologhraphic thermalization Physical quantities that we expect to get: D=5 Ad. S D=4 Minkowski • Black hole formation time • Thermalization time • Entropy • Multiplicity

Thermalization time Experimental data (just estimations) d Holographic estimations Position of horizon ~ size

Thermalization time Experimental data (just estimations) d Holographic estimations Position of horizon ~ size of the trapped surface Bjorken, 1983

Multiplicity Experimental data Plot from: ATLAS Collaboration 1108. 6027 Pb. Pb pp:

Multiplicity Experimental data Plot from: ATLAS Collaboration 1108. 6027 Pb. Pb pp:

Multiplicity as entropy D=4. Macroscopic theory of high-energy collisions Landau(1953); Fermi(1950) thermodynamics, hydrodynamics, kinetic

Multiplicity as entropy D=4. Macroscopic theory of high-energy collisions Landau(1953); Fermi(1950) thermodynamics, hydrodynamics, kinetic theory, … Multiplicity as entropy D=5. Holographic approach Main conjecture: multiplicity ~ entropy of produced D=5 Black Hole Gubser et al: 0805. 1551 The black hole entropy can be estimated by trapped surface area Gubser, Pufu, Yarom, JHEP , 2009 Alvarez-Gaume at al PLB, 2009 IA, Bagrov, Guseva, JHEP, 2009 Kiritsis, Taliotis, JHEP, 2011

Nucleus collision in Ad. S/CFT The metric of two shock waves in Ad. S

Nucleus collision in Ad. S/CFT The metric of two shock waves in Ad. S corresponding to collision of two ultrarelativistic nucleus in 4 D

Multiplicity: Hologhrapic formula vs experimental data

Multiplicity: Hologhrapic formula vs experimental data

Search for models with suitable entropy Metric with modified b-factor IHQCD Reproduces 2 -loops

Search for models with suitable entropy Metric with modified b-factor IHQCD Reproduces 2 -loops QCD beta-function Reproduce an asymptotically-linear glueball spectrum Gursoy, Kiritsis, Nitti

Search for models with suitable entropy Kiritsis, Taliotis, JHEP(2012) Shock wave metric with modified

Search for models with suitable entropy Kiritsis, Taliotis, JHEP(2012) Shock wave metric with modified b-factor Typical behavour not 0. 15

Shock walls collision with modified by b-factor Description of HIC by the wall-wall shock

Shock walls collision with modified by b-factor Description of HIC by the wall-wall shock wave collisions S. Lin, E. Shuryak, 0902. 1508 I. A. , Bagrov and E. Pozdeeva, JHEP(2012) w I. A. , E. Pozdeeva, T. Pozdeeva (2013, 2014) Spoints~swalls

Power-law b-factor Swalls= The multiplicity depends as s 0. 15 NN in the range

Power-law b-factor Swalls= The multiplicity depends as s 0. 15 NN in the range 10 -103 Ge. V Power-law b-factor coinsides with experimental data at a≈0. 47. We consider Price: non standard kinetic term !?

Question: can we fit this background with other data? Multiplicity vs quark potential x[fm]

Question: can we fit this background with other data? Multiplicity vs quark potential x[fm] Ad. S with soft-wall O. Andreev and V. Zakharov hep-ph/0604204 R. Galow at al, 0911. 0627 S. He, M. Huang, Q. Yan 1004. 1880 Coulomb term Confinement linear potential

Multiplicity vs quark potential Soft/hard wall Interpolating geometry? Ad. S 5

Multiplicity vs quark potential Soft/hard wall Interpolating geometry? Ad. S 5

Multiplicity and quark potential with D. Ageev ar. Xiv: 1409. 7558

Multiplicity and quark potential with D. Ageev ar. Xiv: 1409. 7558

Multiplicity and quark potential Trapped surface Pack the trapped surface in the interval But

Multiplicity and quark potential Trapped surface Pack the trapped surface in the interval But restriction on energy Estimation of the termalization time Small energies!

Anisotropy after thermalization In the past: it has been claimed that the preequilibrium period

Anisotropy after thermalization In the past: it has been claimed that the preequilibrium period can only exist for up to 1 fm/c and after that, the QGP becomes isotropic Now: corrections to ideal isotropic behavior even at times ~2 fm/c

Anisotropy after thermalization • Experimental evidence for anisotropies: jet quenching, changes in R-mod. factor,

Anisotropy after thermalization • Experimental evidence for anisotropies: jet quenching, changes in R-mod. factor, photon and dilepton, yields, • QGP is anisotropic for a short time after collision • The time of locally isotropization is about This gives a reason to consider BH formation in anizotropic background

Multiplicity with anisotropic Lifshitz background IA, A. Golubtsova ar. Xiv: 1410. 4595 Shock wave

Multiplicity with anisotropic Lifshitz background IA, A. Golubtsova ar. Xiv: 1410. 4595 Shock wave Solves E. O. M. if

Multiplicity with anisotropic Lifshitz background Domain wall

Multiplicity with anisotropic Lifshitz background Domain wall

Multiplicity with anisotropic Lifshitz background Colliding Domain Walls To get

Multiplicity with anisotropic Lifshitz background Colliding Domain Walls To get

Conclusion Formation of QGP of 4 -dim QCD BH formation in 5 -dim •

Conclusion Formation of QGP of 4 -dim QCD BH formation in 5 -dim • BH formation in isotropic 5 -dim models (Ad. S, b-factor) • b-factor that fits experimental data: 1) Multiplicity 2) Cornell qq-potential • BH formation in Lif. -like 5 -dim models • BH formation in flow from Ad. S to Lif (work in progress)