Dynamical description of heavy-ion collisions Elena Bratkovskaya - - PowerPoint PPT Presentation

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Dynamical description of heavy-ion collisions Elena Bratkovskaya - - PowerPoint PPT Presentation

Dynamical description of heavy-ion collisions Elena Bratkovskaya (GSI, Darmstadt & Uni. Frankfurt) for the PHSD group COST Workshop on Interplay of hard and soft QCD probes for collectivity in heavy-ion collisions 25 February - 1 March


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Dynamical description of heavy-ion collisions

Elena Bratkovskaya

(GSI, Darmstadt & Uni. Frankfurt)

for the PHSD group

COST Workshop on Interplay of hard and soft QCD probes for collectivity in heavy-ion collisions 25 February - 1 March 2019, Lund university, Sweden

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The ‚holy grail‘ of heavy-ion physics:

  • Study of the phase

transition from hadronic to partonic matter – Quark-Gluon-Plasma

  • Search for the critical point
  • Study of the in-medium properties of hadrons

at high baryon density and temperature The phase diagram of QCD

  • Search for signatures of

chiral symmetry restoration

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Theory: Information from lattice QCD

  • II. chiral symmetry restoration

with increasing temperature

  • I. deconfinement phase transition

with increasing temperature

+

 both transitions occur at about the same temperature TC for low chemical potentials

lQCD BMW collaboration:

T s l,

q q q q ~ Δ

 Crossover: hadron gas  QGP  Scalar quark condensate is viewed as an order parameter for the restoration

  • f chiral symmetry:

mq=0

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Degrees-of-freedom of QGP

 lQCD gives QGP EoS at finite mB pQCD:  weakly interacting system  massless quarks and gluons Thermal QCD = QCD at high parton densities:  strongly interacting system  massive quarks and gluons  quasiparticles = effective degrees-of-freedom ! need to be interpreted in terms of degrees-of-freedom

Non-perturbative QCD  pQCD

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Theory  HIC experiments

 How to learn about degrees-of- freedom of QGP?

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  • Statistical models:

basic assumption: system is described by a (grand) canonical ensemble of non-interacting fermions and bosons in thermal and chemical equilibrium = thermal hadron gas at freeze-out with common T and mB

[ - : no dynamical information]

  • Hydrodynamical models:

basic assumption: conservation laws + equation of state (EoS); assumption of local thermal and chemical equilibrium

  • Interactions are ‚hidden‘ in properties of the fluid described by transport coefficients

(shear and bulk viscosity h, z, ..), which is ‘input’ for the hydro models

[ - : simplified dynamics]

  • Microscopic transport models:

based on transport theory of relativistic quantum many-body systems

  • Explicitly account for the interactions of all degrees of freedom (hadrons and partons)

in terms of cross sections and potentials

  • Provide a unique dynamical description of strongly interaction matter

in- and out-off equilibrium:

  • In-equilibrium: transport coefficients are calculated in a box – controled by lQCD
  • Nonequilibrium dynamics – controled by HIC

Actual solutions: Monte Carlo simulations

[+ : full dynamics | - : very complicated]

Basic models for heavy-ion collisions

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History: Semi-classical BUU equation

coll p r r

t f ) t , p , r ( f ) t , r ( U ) t , p , r ( f m p ) t , p , r ( f t                           

  

Boltzmann-Uehling-Uhlenbeck equation (non-relativistic formulation)

  • propagation of particles in the self-generated Hartree-Fock mean-field

potential U(r,t) with an on-shell collision term:

) term Fock ( ) t , p , r ( f ) t , r r ( V p d r d ) 2 ( 1 ) t , r ( U

3 3 3

  • cc

     



     

) t , p , r ( f  

is the single particle phase-space distribution function

  • probability to find the particle at position r with momentum p at time t

 self-generated Hartree-Fock mean-field potential:

Ludwig Boltzmann

collision term: elastic and inelastic reactions

P ) 4 3 2 1 ( d d ) p p p p ( | | d p d p d ) 2 ( 4 I

4 3 2 1 3 12 3 3 2 3 3 coll

        

 

         

Probability including Pauli blocking of fermions:

) f 1 )( f 1 ( f f ) f 1 )( f 1 ( f f P

4 3 2 1 2 1 4 3

     

Gain term: 3+41+2 Loss term: 1+23+4  Collision term for 1+23+4 (let‘s consider fermions) : 1 2 3 4

t 

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Elementary hadronic interactions

Low energy collisions:

  • binary 22 and

23(4) reactions

  • 12 : formation and

decay of baryonic and mesonic resonances BB  B´B´ BB  B´B´m mB  m´B´ mB  B´ mm  m´m´ mm  m´ . . . Baryons: B = p, n, (1232), N(1440), N(1535), ... Mesons: M = , h, r, w, f, ...

+p pp

High energy collisions: (above s1/2~2.5 GeV) Inclusive particle production: BBX , mBX, mmX X =many particles described by string formation and decay (string = excited color singlet states q-qq, q-qbar) using LUND string model Consider all possible interactions – eleastic and inelastic collisions - for the sytem

  • f (N,R,m), where N-nucleons, R- resonances, m-mesons, and resonance decays

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From weakly to strongly interacting systems

Many-body theory: Strong interaction  large width = short life-time  broad spectral function  quantum object

  • How to describe the dynamics of

broad strongly interacting quantum states in transport theory?

Barcelona / Valencia group L(1783)N-1 and S(1830)N-1 exitations

 semi-classical BUU  generalized transport equations based on Kadanoff-Baym dynamics first order gradient expansion of quantum Kadanoff-Baym equations

In-medium effects (on hadronic or partonic levels!) = changes of particle properties in the hot and dense medium Example: hadronic medium - vector mesons, strange mesons QGP – dressing of partons

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Dynamical description of strongly interacting systems

 Semi-classical on-shell BUU: applies for small collisional width, i.e. for a weakly

interacting systems of particles

 Quantum field theory 

Kadanoff-Baym dynamics for resummed single-particle Green functions S< (1962)

Leo Kadanoff Gordon Baym

) M ( S ˆ

2 x x 1 x

    

 m m

advanced S S S S S retarded S S S S S

a xy xy xy c xy adv xy a xy xy xy c xy ret xy

         

   

anticausal } ) y ( Φ ) x ( {Φ T iS causal } ) y ( Φ ) x ( {Φ T iS } ) x ( Φ ) y ( {Φ iS } ) x ( Φ ) y ( {Φ η iS

a a xy c c xy xy xy

             

     

Green functions S< / self-energies S:

  • perator
  • rdering

time ) anti ( ) T ( T ) fermions / bosons ( 1

c a

     h

Integration over the intermediate spacetime

How to describe strongly interacting systems?!

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From Kadanoff-Baym equations to generalized transport equations

After the first order gradient expansion of the Wigner transformed Kadanoff-Baym equations and separation into the real and imaginary parts one gets: Backflow term incorporates the off-shell behavior in the particle propagation ! vanishes in the quasiparticle limit AXP  (p2-M2)  Spectral function: – ‚width‘ of spectral function = reaction rate of particle (at space-time position X)

4-dimentional generalizaton of the Poisson-bracket:

  • W. Cassing , S. Juchem, NPA 665 (2000) 377; 672 (2000) 417; 677 (2000) 445

 GTE: Propagation of the Green‘s function iS<XP=AXPNXP , which carries

information not only on the number of particles (NXP), but also on their properties, interactions and correlations (via AXP)  S 

ret XP XP

p 2 Im   

drift term Vlasov term collision term = ‚gain‘ - ‚loss‘ term backflow term

Generalized transport equations (GTE):

  c    Life time

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General testparticle off-shell equations of motion

 Employ testparticle Ansatz for the real valued quantity i S<

XP

insert in generalized transport equations and determine equations of motion !

 General testparticle Cassing‘s off-shell equations of motion for the time-like particles:

with

  • W. Cassing , S. Juchem, NPA 665 (2000) 377; 672 (2000) 417; 677 (2000) 445
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Collision term in off-shell transport models

Collision term for reaction 1+2->3+4: with The trace over particles 2,3,4 reads explicitly for fermions for bosons

The transport approach and the particle spectral functions are fully determined once the in-medium transition amplitudes G are known in their off-shell dependence!

additional integration ‚loss‘ term ‚gain‘ term

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Goal: microscopic transport description of the partonic and hadronic phase

Problems:

 How to model a QGP phase in line with lQCD data?

 How to solve the hadronization problem?

Ways to go:

‚Hybrid‘ models:

  • QGP phase: hydro with QGP EoS
  • hadronic freeze-out: after burner -

hadron-string transport model  Hybrid-UrQMD

  • microscopic transport description of the partonic

and hadronic phase in terms of strongly interacting dynamical quasi-particles and off-shell hadrons  PHSD pQCD based models:

  • QGP phase: pQCD cascade
  • hadronization: quark coalescence

 AMPT, HIJING, BAMPS

16

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From SIS to LHC: from hadrons to partons

The goal: to study of the phase transition from hadronic to partonic matter and properties of the Quark-Gluon-Plasma from a microscopic origin  need a consistent non-equilibrium transport model  with explicit parton-parton interactions (i.e. between quarks and gluons)  explicit phase transition from hadronic to partonic degrees of freedom  lQCD EoS for partonic phase (‚crossover‘ at small mq)

Parton-Hadron-String-Dynamics (PHSD)

QGP phase described by Dynamical QuasiParticle Model (DQPM)

 Transport theory: off-shell Kadanoff-Baym equations for the

Green-functions S<

h(x,p) in phase-space representation for the

partonic and hadronic phase

  • A. Peshier, W. Cassing, PRL 94 (2005) 172301;

Cassing, NPA 791 (2007) 365: NPA 793 (2007)

  • W. Cassing, E. Bratkovskaya, PRC 78 (2008) 034919;

NPA831 (2009) 215;

  • W. Cassing, EPJ ST 168 (2009) 3
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DQPM describes QCD properties in terms of ‚resummed‘ single-particle Green‘s functions (propagators) – in the sense of a two-particle irreducible (2PI) approach:

  • A. Peshier, W. Cassing, PRL 94 (2005) 172301; Cassing, NPA 791 (2007) 365: NPA 793 (2007)

Dynamical QuasiParticle Model (DQPM) - Basic ideas:

  • the resummed properties are specified by complex (retarded) self-energies:
  • the real part of self-energies (Σq, Π) describes a dynamically generated mass (Mq,Mg);
  • the imaginary part describes the interaction width of partons (gq, gg)
  • Spectral functions :

(scalar approximation)

gluon self-energy: Π=Mg2-i2ggω & quark self-energy: Σq=Mq2-i2gqω gluon propagator: Δ-1 =P2 - Π & quark propagator Sq

  • 1 = P2 - Σq

ret g ret q q

Im A ~ImS A  ~ ,

 Entropy density of interacting bosons and fermions in the quasiparticle limit (2PI)

gluons quarks antiquarks

QGP

(G. Baym 1998):

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DQPM(T,mq): properties of quasiparticles

Properties of interacting quasi-particles: massive quarks and gluons (g, q, qbar) with Lorentzian spectral functions :

Peshier, Cassing, PRL 94 (2005) 172301; Cassing, NPA 791 (2007) 365: NPA 793 (2007)

with 3 parameters: Ts/Tc=0.46; c=28.8; l=2.42 (for pure glue Nf=0)

 fit to lattice (lQCD) results (e.g. entropy density)

  • running coupling (pure glue):

lQCD: pure glue

  • Modeling of the quark/gluon masses and widths  HTL limit at high T

masses: widths:

2 2 2 2

g    M p E

m~gT

for mq=0

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DQPM at finite T and mq

Peshier, Cassing, PRL 94 (2005) 172301; Cassing, NPA 791 (2007) 365: NPA 793 (2007)

 Quasiparticle properties:

  • large width and mass for gluons and quarks
  • fit to lattice (lQCD) results

* BMW lQCD data S. Borsanyi et al., JHEP 1009 (2010) 073

TC=158 MeV eC=0.5 GeV/fm3

mq=0

 microscopic dynamical transport approach PHSD masses widths

M~gT

DQPM

  • matches well lattice QCD
  • provides mean-fields (1PI) for gluons and

quarks – from space-like part of Tmn as well as effective 2-body interactions (2PI)

  • gives transition rates for the formation of hadrons

mq=0

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 Formation of QGP stage if e > ecritical :

dissolution of pre-hadrons  (DQPM)   massive quarks/gluons + mean-field potential Uq

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Parton-Hadron-String-Dynamics (PHSD)

 Hadronic phase: hadron-hadron interactions – off-shell HSD

  • W. Cassing, E. Bratkovskaya, PRC 78 (2008) 034919; NPA831 (2009) 215; W. Cassing, EPJ ST 168 (2009) 3

 Initial A+A collisions : N+N  string formation  decay to pre-hadrons

g g g g g q q     

  • (quasi-) elastic collisions:
  • inelastic collisions:

q q g g q q    

q q q q q q q q q q q q          g g g g q g q g q g q g         

 Partonic stage – QGP :

based on the Dynamical Quasi-Particle Model (DQPM)

) ' string '

  • r

( baryon q q q ) ' string '

  • r

( meson q q , q q g         Hadronization (based on DQPM):

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QGP in equilibrium: Transport properties at finite (T, mq): h/s

Shear viscosity h/s at finite (T, mq) Shear viscosity h/s at finite T

PHSD: V. Ozvenchuk et al., PRC 87 (2013) 064903 Hydro: Bayesian analysis, S. Bass et al. ,1704.07671

h/s: mq=0  finite mq: smooth increase as a function of (T, mq)

Review: H. Berrehrah et al. Int.J.Mod.Phys. E25 (2016) 1642003

Infinite hot/dense matter = PHSD in a box: QGP in PHSD = strongly- interacting liquid-like system lQCD:

DQPM

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Traces of the QGP in observables in high energy heavy-ion collisions

http://theory.gsi.de/~ebratkov/phsd-project/PHSD/index1.html

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Pierre Moreau

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Stages of a collision in PHSD

Traces of non-equilibrium dynamics in relativistic heavy-ion collisions

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Pierre Moreau

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Traces of non-equilibrium dynamics in relativistic heavy-ion collisions

Stages of a collision in PHSD

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Pierre Moreau

11

Traces of non-equilibrium dynamics in relativistic heavy-ion collisions

Stages of a collision in PHSD

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Pierre Moreau

11

Traces of non-equilibrium dynamics in relativistic heavy-ion collisions

Stages of a collision in PHSD

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Pierre Moreau

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Traces of non-equilibrium dynamics in relativistic heavy-ion collisions

Stages of a collision in PHSD

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Pierre Moreau

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Traces of non-equilibrium dynamics in relativistic heavy-ion collisions

Stages of a collision in PHSD

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Partonic energy fraction in central A+A

 Strong increase of partonic phase with energy from AGS to RHIC  SPS: Pb+Pb, 160 A GeV: only about 40% of the converted energy goes to partons; the rest is contained in the large hadronic corona and leading partons  RHIC: Au+Au, 21.3 A TeV: up to 90% - QGP

  • W. Cassing & E. Bratkovskaya, NPA 831 (2009) 215
  • V. Konchakovski et al., Phys. Rev. C 85 (2012) 011902

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Time evolution of the partonic energy fraction vs energy

Au+Au, midrapidity

  • T. Steinert et al.
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Transverse mass spectra from SPS to RHIC

Central Pb + Pb at SPS energies

 PHSD gives harder mT spectra and works better than HSD (wo QGP) at high energies

– RHIC, SPS (and top FAIR, NICA)  however, at low SPS (and low FAIR, NICA) energies the effect of the partonic phase decreases due to the decrease of the partonic fraction

Central Au+Au at RHIC

  • W. Cassing & E. Bratkovskaya, NPA 831 (2009) 215
  • E. Bratkovskaya, W. Cassing, V. Konchakovski, O. Linnyk, NPA856 (2011) 162

35

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Elliptic flow v2 vs. collision energy for Au+Au

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  • v2 in PHSD is larger than in HSD due

to the repulsive scalar mean-field potential Us(ρ) for partons

  • v2 grows with bombarding energy due

to the increase of the parton fraction

  • V. Konchakovski, E. Bratkovskaya, W. Cassing, V. Toneev,
  • V. Voronyuk, Phys. Rev. C 85 (2012) 011902

with QGP without QGP

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Vn (n=2,3,4,5) of charged particles from PHSD at LHC

  • V. Konchakovski, W. Cassing, V. Toneev, J. Phys. G: Nucl. Part. Phys 42 (2015) 055106
  • PHSD: increase of vn (n=2,3,4,5) with pT
  • v2 increases with decreasing centrality
  • vn (n=3,4,5) show weak centrality dependence

symbols – ALICE

PRL 107 (2011) 032301

lines – PHSD (e-by-e)

vn (n=3,4,5) develops by interaction in the QGP and in the final hadronic phase

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T s l,

q q q q ~ Δ

Problem: K+/+ ‚horn‘ – 2015

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PHSD: even when considering the creation of a QGP phase, the K+/+ ‚horn‘ seen experimentally by NA49 and STAR at a bombarding energy ~30 A GeV (FAIR/NICA energies!) remains unexplained !

 The origin of ‘horn’ is not traced back to deconfinement ?!

  • W. Cassing, A. Palmese, P. Moreau, E.L. Bratkovskaya, PRC 93, 014902 (2016)

Can it be related to chiral symmetry restoration in the hadronic phase?!

lQCD BMW collaboration:

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Chiral symmetry restoration vs. deconfinement

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  • I. Initial stage of HIC collisions:

Hadronic matter  string formation QGP

I II

  • II. QGP III. Hadronic phase

(time-like partons, explicit partonic interactions) Hadronic matter

QGP

               g 2 exp ) ( ) ( ) ( ) (

2 * 2 * q S S

m m d d P s s P u u P s s P

V q V q

m m        q q q q ) ( m m

q * q

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Excitation function of hadron ratios and yields

33  Influence of EoS: NL1 vs NL3  low sensitivity to the nuclear EoS  Excitation function of the hyperons LS0 and X show analogous peaks as K+/+, (LS0)/ ratios due to CSR

  • A. Palmese et al., PRC94 (2016) 044912 , arXiv:1607.04073

Chiral symmetry restoration leads to the enhancement of strangeness production in string fragmentation in the beginning of HIC in the hadronic phase

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Summary

Microscopic transport approach PHSD versus experimental observables:  evidence for strong partonic interactions in the early phase of relativistic heavy-ion reactions  indication for a partial chiral symmetry restoration

formation of the sQGP in HIC!

http://theory.gsi.de/~ebratkov/phsd-project/PHSD/index1.html

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GSI & Frankfurt University Elena Bratkovskaya Pierre Moreau Lucia Oliva Olga Soloveva Giessen University Wolfgang Cassing Taesoo Song Thorsten Steinert Alessia Palmese Eduard Seifert

External Collaborations

SUBATECH, Nantes University: Jörg Aichelin Christoph Hartnack Pol-Bernard Gossiaux Marlene Nahrgang Texas A&M University: Che-Ming Ko JINR, Dubna: Viacheslav Toneev Vadim Voronyuk Viktor Kireev Valencia University: Daniel Cabrera Barcelona University: Laura Tolos Duke University: Steffen Bass

Thanks to: PHSD group - 2019

Thanks to Olena Linnyk Volodya Konchakovski Hamza Berrehrah

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Thank you for your attention ! Thanks to the Organizers !