What is the bulk viscosity Of QCD matter? - …mstrick6/qcdseminar/spring16/denicol.pdf ·...
Transcript of What is the bulk viscosity Of QCD matter? - …mstrick6/qcdseminar/spring16/denicol.pdf ·...
with:
J.F. Paquet, S. Ryu, C. Shen, B. Schenke, S. Jeon, C. Gale
Kent State University 10.March.2016
What is the bulk viscosity
Of QCD matter?
Gabriel S. Denicol (BNL)
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Shear viscosity of QCD matter exhibits surprising features near phase transition region
What about bulk viscosity?
“h/s”
3
What is bulk viscosity?
Non-equilibrium contribution to pressure Pressure =
thermodynamicpressure
> 0 < 0
Resistance to expansion
Resistance to compression
(Shock waves)(HIC,universe)
“dP”
4
Shear viscosity
Resistance to deformation
Sources of viscosity and dissipation
Resistance to volume change
Bulk viscosity
5
Bulk to shear viscosity ratio for several gases
Some known examples
In many cases, bulk viscosity can be larger than shear viscosity
M. Cramer, Phys. of fluids 24, 066102 (2012)
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Bulk to shear viscosity ratio for several gases
Some known examples
M. Cramer, Phys. of fluids 24, 066102 (2012)
Comment: bulk viscosity from non-relativistic Boltzmann equation is zero
7
pions gas pQCD
Bulk viscosity ~1000 times smaller than shear
What about nuclear matter?some understood limits
Arnold et al, PRD 74, 085021 (2006)
Prakash et al, Phys. Rept. 227, 321 (1993)
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QCD is not conformal
Lattice QCD calculations demonstrate that the EoS
of QCD matter deviates from that of a conformal fluid
Bulk viscosity couldbecome large in this
region
Near phase transition? we do not know
?
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Initial state
Pre-equilibriumdynamics
QGP as a relativisticfluid
Hadronization Transport/Freezeout
0 ~1 ~10
fm/c
~20
Ultra-relativistic Heavy Ion Collisions
Best (and often only) option to understand certainproperties of bulk nuclear matter
MADAI collaboration
Goal: use all data available to extract transport properties of QCD matter & understand initial state
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Initial state
Pre-equilibriumdynamics
QGP as a relativisticfluid
Hadronization Transport/Freezeoutfm/c
Bulk QCD matter is only created transientlyNeed to reverse-engineer its properties
MADAI collaboration
Very large expansion rate! If bulk is sufficientlylarge, it should be possible to see it.
0 ~1 ~10 ~20
Ultra-relativistic Heavy Ion Collisions
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Extraction of shear viscosityShear viscosity can be estimated using elliptic
flow data
Song et al, PRL 106, 192301 (2011)
The QGP is an almost perfect fluid with a shear viscosity ~10 times smaller than predictions from pQCD
14
Extraction of shear viscosity
IP-Glasma model offered a very good descriptionof flow harmonics
Gale et al, PRL 110, 1, 012302 (2013)
Shear viscosity can be estimated using elliptic and triangular flow data
15
Strong correlation between flow harmonics and initial geometry
shear viscosity reduces the hydrodynamic response to the initial gradients
provides good way toextract shear viscosity
16
What you will see in this talk
We investigate the effect of bulk viscosity on basic heavy ion collision observables
✔ Does bulk viscosity have a considerable effect on basic heavy ion observables? Is it needed to fit the data?
✔ Can it be extracted? What observable should we use?
✔ Does the inclusion of bulk viscosity change our current understanding of the transport properties of the QGP?
Questions addressed:
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Hydrodynamic modeling of heavy ion collisions
Initial state and pre-equilibrium dynamics description of early time-dynamics and thermalization
IP-Glasma “initial condition”
Fluid-dynamical expansion of QGP and Hadron Gas
Transport description of Hadron Gas Matter described by cross sections and decay probabilities
UrQMD
thermalization “by hand”
fluid elements convertedto particles
EoS, viscosities, ...
+ EoM for dissipative currents
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Fluid-dynamical equations
Inclusion of bulk viscous pressure, shear-stress tensor, and all couplings
GSD&Niemi&Molnar&Rischke, PRD 85, 114047 (2012)
For collisions at lower energies, baryon number diffusion is also included
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✔ Switching to UrQMD at T=const.
✔ We solve the fluid-dynamical equations using a relativistic version of the KT algorithm – MUSIC
✔ lQCD + HRG EoS by Huovinen&Petrescky
✔ IP-Glasma initial state, t0 = 0.4 fm
SimulationIP-Glasma+MUSIC+UrQMD
PRL 115, 132301 (2015)
✔ h/s=const, ✔ z/s =
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Integrated observables Tswitch = 145 MeV h/s = 0.095
bulk viscosity increases multiplicity, reduces <pT>, and reduces Vn
Surprisingly large effects of bulk viscosity
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Integrated observables Tswitch = 145 MeV
bulk viscosity increases multiplicity, reduces <pT>, and reduces Vn
Value of shear viscosity extracted changes significantlyh/s=0.16 0.095
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Effect of switching temperature
With only shear: changing Tsw is not enough to fit the data
Shear only
h/s=0.16
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Effect of switching temperature
With bulk: fitting the data becomes possible
Shear + bulk
h/s=0.095
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Effect of re-scatterings
Effect of re-scatterings is significantfor kaons and protons
<pT> is affected significantly
Tswitch = 145 MeV h/s = 0.095
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Same conclusions remainWhat about RHIC?
h/s=0.06 Tswitch=165 MeV
Same bulk viscosity can also describe RHIC data
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Results from Duke group
Model: Trento initial state + Hydro (bulk&shear) + UrQMD
shear not well constrained with just LHC datafinite bulk viscosity is favored
Similar findings also by Schenke&Monnai for MC-Glauber with valence quarks
Very good description of Multiplicity, mean-pT, and Vn
p
K
p
X
LHC 2.76 TeV, 0-5%MUSIC + UrQMDALICE data
0 10 20 30 40Centrality (%)
0.1
1
10
100
1000
10000
dN/d
y
(L+S0)/2
W
Hadron chemistry is reasonably described
0.4 0.8 1.2 1.6 2pT (GeV)
0
0.05
0.1
0.15
0.2
v n{2
}
0.4 0.8 1.2 1.6 2pT (GeV)
0.4 0.8 1.2 1.6 2pT (GeV)
1
10
100
1000
10000
1/2
dN
/pTdp
T
LHC 2.76 TeV, 0-5%MUSIC + UrQMDALICE data
LHC 2.76 TeV, 10-20%MUSIC + UrQMDALICE data
LHC 2.76 TeV, 20-30%MUSIC + UrQMDALICE data
n=2n=3
n=4
p
K
p
p
K
p
p
K
p
n=2
n=3
n=4
n=2
n=3
n=4
1/(2
ppT) d
N/d
p T
charged hadrons charged hadrons charged hadrons
Overall description of differential observables
Vn coefficients – different pT cuts
Good agreement at low pTDisagreement with data starts at high pT
1 2 3 4 5 6n
0.001
0.01
0.1
Pb+Pb, 2.76 TeV, 10-20%ATLAS data0.5< pT< 1.0 GeV
1.0< pT< 2.0 GeV
2.0< pT< 3.0 GeV
1 2 3 4 5 6n
0.001
0.01
0.1
Pb+Pb, 2.76 TeV, 20-30%ATLAS data0.5< pT< 1.0 GeV
1.0< pT< 2.0 GeV
2.0< pT< 3.0 GeV
v n{2
}
HBT radius – calculation by C. Shen et al
Good description of HBT
Bulk helps a little, butthis is mainly due to
the inclusion of UrQMD
Transverse momentum distribution
Protons: we describe STAR data, but not PHENIX!
0 0.4 0.8 1.2 1.6 2pT (GeV)
0
0.04
0.08
0.12
0.16
0.2
RHIC 200 GeV, 10-20%MUSIC + UrQMDPHENIX data
v2{4}
v3{2}
v4{2}
Good description of differential observables
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EKRT model + second order viscous hydroNiemi et al, PRC 93, no. 2, 024907 (2016)
Good description without including bulk viscosity!But, chemical freeze-out at 175 MeV
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Non-equilibrium contribution to pressure Pressure =
“dP”
Hydrodynamical picture works, if this is a perturbative correction to the thermodynamic pressure
PPCE = P0 + dP
Different descriptions of the same effect?
bulk?
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IP-Glasma + MUSIC + UrQMD LHCz/s(T) h/s=0.095Ryu et al, PRL 115, 132301 (2015)
IP-Glasma initial conditions lead to
high mean pT
Bulk viscosityreduces mean
pT
PRL 115, 132301 (2015)
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Evolution of initial state
Smooth Initial conditions(v2=0 in central collisions)
Fluctuations in nucleon positions(odd harmonics)
sub-nucleonic fluctuations (vn distributions&correlations)
proton-nucleus collisions
l~5 fm
l~1 fm
l~0.4 fm
l~0.4 fmor smaller
e(x,y) Coarse-grainingsize
IP-Glasma event
l = 0.1 fm l = 0.2 fm
l = 0.4 fm l = 0.8 fm l = 1.6 fm
0-5% class
Effect of smoothing
0.4 0.8 1.2 1.6(fm)
0.3
0.35
0.4
0.45
0.5<
p T>
shear only
shear+bulk
data
Effect of initial thermalization scale
p (G
eV)
Correlation to initial thermalization scale
L (fm)
shear only
<L>-1 = <e>/<e>
<pT> ~ <L>-1
<p T
> (
GeV
) p
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Summary/conclusions
We studied the effect of bulk viscosity the transverse momentum spectra and azimuthal
momentum anisotropies
✔ Bulk viscosity has a considerable effect on multiplicity, transverse momentum, and flow harmonics
✔ For IP-Glasma initial conditions, bulk viscosity improves the agreement between theory and experiment
✔ The mean transverse momentum is linearly related to the initial energy density gradients
It should be possible to extract it
Nk/Np
0 0.4 0.8 1.2 1.6 2pT (GeV)
0
0.2
0.4
0.6
0.8
LHC 2.76 TeV, 10-20%MUSIC + UrQMDALICE data
0 0.4 0.8 1.2 1.6 2pT (GeV)
0
0.2
0.4
0.6
0.8
LHC 2.76 TeV, 30-40%MUSIC + UrQMDALICE data
Np/Np
Nk/Np
Np/Np
Particle ratios
Pion to proton ratio is well describedKaons are slightly over-predicted
0.4 0.8 1.2 1.6 2pT (GeV)
0
0.1
0.2
0.3
v 2{2}
LHC 2.76 TeV, 20-30%MUSIC + UrQMDALICE data
0.4 0.8 1.2 1.6 2pT (GeV)
0
0.1
0.2
0.3
v 2{2}
LHC 2.76 TeV, 10-20%MUSIC + UrQMDALICE data
p
pK
p
pK
Diffential elliptic flow
Reasonable descriptionUrQMD is an important factor for this
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Bulk viscosity from kinetic theory
Weinberg (matter coupled to radiation)
Dusling&Schaefer (pure glue)
14-moment approximation (Anderson-Witting equation)
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Model: IP-Glasma + MUSIC (bulk&shear)
large bulk viscosity around “Tc” is favored by dataConsistent with our previous findings (recently confirmed by Duke group)
Extraction of z/s(T) and h/s with MADAI Emulator
z/s(T) parametrized as a Breit-Wigner distribution
0.4 0.8 1.2 1.6T/Tc
0
0.1
0.2
0.3
0.4
0.5
Parameters extracted
z/s(T) band = 1 sigma
“Tc” = 0.177 0.022 GeV+-
h/s = 0.077 0.037+-
LHC energy
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h/s
z/s(Tc)
non-conformal holographyprediction
Correlation between Bulk and Shear
Increasing z/s leads to a reduction of h/s flow harmonics
Value of z ismuch larger than expectedFinazzo et al, arXiv:1412.2968
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Event-by-event fluctuations changed the game
Centrality dependence of vnv2 distributions (measured by ATLAS)
PhD thesis of C. Shen Renk&Niemi, PRC 89 (2014) 6, 064907
Cannot be described by Glauber and KLN
Difficult to describe
v2 and v
3 with the
same shear viscosity
Hydrodynamic models should describe, not only event-averaged observables, but also distributions/correlations of observables
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IPsat model + Yang-Mills evolution IP-Glasma:
Gale et al, PRL 110 (2013) 1, 012302
Schenke et al, PRC86 (2012) 034908
h/s=0.2
Very good description of flow harmonic coefficients
Prediction of vn distribution