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The quest for the holy Grail: from Glasma to Plasma Raju Venugopalan CATHIE-TECHQM workshop, Dec. 14-18, 2009 Color Glass Condensates Initial Singularity Glasma sQGP - perfect fluid Hadron Gas t

The quest for the holy Grail: from Glasma to Plasma Raju Venugopalan CATHIE-TECHQM workshop, Dec. 14-18, 2009 Color Glass Condensates Initial Singularity

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Page 1: The quest for the holy Grail: from Glasma to Plasma Raju Venugopalan CATHIE-TECHQM workshop, Dec. 14-18, 2009 Color Glass Condensates Initial Singularity

The quest for the holy Grail: from Glasma to Plasma

Raju Venugopalan

CATHIE-TECHQM workshop, Dec. 14-18, 2009

Color Glass

Condensates

Initial

Singularity

Glasma sQGP - perfect fluid

Hadron Gas

t

Page 2: The quest for the holy Grail: from Glasma to Plasma Raju Venugopalan CATHIE-TECHQM workshop, Dec. 14-18, 2009 Color Glass Condensates Initial Singularity

Nuclear wavefunction at high energies

At RHIC typical x ~ 0.01 . At the LHC, x ~ 5 * 10-4

PartonDensity

x= fraction of momentum of hadron carried by parton

Glue rules!

For glue, QS

2 = 1-1.4 GeV2 (RHIC)QS

2 = 2.6-4 GeV2 (LHC)

Kowalski,Lappi,RV, PRL (2008)

Nuclear wave function at high energies is a Color Glass Condensate

Page 3: The quest for the holy Grail: from Glasma to Plasma Raju Venugopalan CATHIE-TECHQM workshop, Dec. 14-18, 2009 Color Glass Condensates Initial Singularity

CGC: effective degrees of freedom

Fields Sources

x 1

Time dilated, “frozen” random color charges with weight W[]

Dynamical gauge fields

Classical eqns: RG eqn. for x evolution of source dist.: resums Sln(1/x) and /kT

2 contributions in loop corrections

Saturation scale QS: Non.Pert. scale in W at x0 grows with x evol. of RG

Page 4: The quest for the holy Grail: from Glasma to Plasma Raju Venugopalan CATHIE-TECHQM workshop, Dec. 14-18, 2009 Color Glass Condensates Initial Singularity

From CGC to Glasma

Multi-particle production from strong CGC fields:compute systematically properties of strongly correlated Glasma fields after collision

Consider T : At LO, can obtain from soln. of classical Yang-Mills eqns.

NLO terms are as large as LO for S ln(1/x) - resum to all ordersGelis,Lappi,RV (2008)

Glasma factorization => universal “density matrices W” calc. “matrix element”

Page 5: The quest for the holy Grail: from Glasma to Plasma Raju Venugopalan CATHIE-TECHQM workshop, Dec. 14-18, 2009 Color Glass Condensates Initial Singularity

<T> in the GlasmaAt RHIC energies, in central A+A, evolution of W’s is not significant - local Gaussian dist. of sources with variance QS

2 ; at LHC, evolution is very significantKrasnitz,Nara,RV (2003)

System initially very far from equilibrium! (Tzz <0 for =0+ and ->0 for > 1/QS)

Lappi,McLerran (2006)

Initial gauge field configurations are longitudinal chromo-electric & magnetic fields localized in transverse plane

- generate Chern-Simons charges0Kharzeev,Krasnitz,RV (2002)

Page 6: The quest for the holy Grail: from Glasma to Plasma Raju Venugopalan CATHIE-TECHQM workshop, Dec. 14-18, 2009 Color Glass Condensates Initial Singularity

Glasma flux tubes-IDumitru,Gelis,McLerran,RV (2008)

Conjecture based on pert. calculation:Glasma is a collection of “flux tubes” color screened on transverse distances ~ 1/QS

If conjecture is true, from geometry, must have

Non-perturbative (soln. of classical QCD!) computation of double inclusive gluon production in Glasma Lappi,Srednyak,RV:arXiv 0911.2068

Page 7: The quest for the holy Grail: from Glasma to Plasma Raju Venugopalan CATHIE-TECHQM workshop, Dec. 14-18, 2009 Color Glass Condensates Initial Singularity

Glasma flux tubes-II

Three possible scales for color screening: 1/R, m (QCD), QS

For 2 =1, (0.5-2) QS2

Color screening radius ~ 0.7-1.4 QS

Quantum evolution of distributions will give additional screening

Results of non-pert. computation confirm Glasma flux tube conjecture

Flux tube size in same ball park as experiments. Some variation in value depending on observable

Iancu,Itakura,McLerran (2002)A.H.Mueller (2003)

Long range rapidity correlations -> see Dusling talkarXiv:0911.2720

Page 8: The quest for the holy Grail: from Glasma to Plasma Raju Venugopalan CATHIE-TECHQM workshop, Dec. 14-18, 2009 Color Glass Condensates Initial Singularity

Matching Glasma dynamics to Hydro

Classical fieldClassical field / Particle Particle

f < 1

Current matching of LO Glasma YM computations to hydro - “CGC initial conditions”- assumes instantaneous thermalization

But T is far out of equilibrium in LO computations

No computations to date fully take into account NLO contributions that are as large as LO and should be resummed…

eccentricity

Page 9: The quest for the holy Grail: from Glasma to Plasma Raju Venugopalan CATHIE-TECHQM workshop, Dec. 14-18, 2009 Color Glass Condensates Initial Singularity

Unstable quanta in the GlasmaRomatschke,RV (2006)

Boost non-invariant quantum fluctuations can grow rapidlyfor > 0

for

Strong disordering could lead to rapid isotropization, “anomalous transport”

Asakawa,Bass,Muller (2006)Dumitru,Nara,Schenke,Strikland (2008)These quantum corrections, albeit difficult to

evaluate, are no less a necessary partof early time dynamics…

3+1-D YM simulations

Page 10: The quest for the holy Grail: from Glasma to Plasma Raju Venugopalan CATHIE-TECHQM workshop, Dec. 14-18, 2009 Color Glass Condensates Initial Singularity

Rapid isotropization in the Glasma

Resum - extend range of YM-dynamics

“Holy Grail” Spectrum of small fluctuations

Fukushima,Gelis,McLerran (2006)

Gelis,Lappi,RV (2008)

Can also compute event by event initial conditions to estimate flow fluctuations:

Similar in spirit to the event by event hydro code

NeXSPheRIO = NeXus + SPheRIO Grassi et al., arXiv:0912.0703

Page 11: The quest for the holy Grail: from Glasma to Plasma Raju Venugopalan CATHIE-TECHQM workshop, Dec. 14-18, 2009 Color Glass Condensates Initial Singularity

Summary

The early time dynamics of HI collisions can be computed ab initio in a factorization framework

Early time Yang-Mills dynamics reveals structure of the Glasma as a collection of flux tubes color screened on distances ~ 1/QS

Quantum instabilities from the wave-function can lead to early isotropization; significant effects on final states

The factorization framework for n-point correlations is ideally suited to event-by-event analysis

Many interesting conceptual issues in understanding the Glasma -> sQGP transition