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The properties of parton- -hadron matter hadron matter The - - PowerPoint PPT Presentation

The properties of parton- -hadron matter hadron matter The properties of parton from heavy- -ion collisions ion collisions from heavy Elena lena Bratkovskaya Bratkovskaya E Institut f r Theoretische Physik r Theoretische Physik


slide-1
SLIDE 1

1 1

The properties of parton The properties of parton-

  • hadron matter

hadron matter from heavy from heavy-

  • ion collisions

ion collisions

E Elena lena Bratkovskaya Bratkovskaya

Institut f Institut fü ür Theoretische Physik r Theoretische Physik & FIAS, Uni. Frankfurt & FIAS, Uni. Frankfurt

BLTP, BLTP, 7 August, 2013 7 August, 2013

slide-2
SLIDE 2

2 2

From Big Bang to Formation of the Universe

  • Can we go back in time ?

time

3 min nucleons deuterons α α α α− − − −particles 10-3sec quarks gluons photons

T~160 MeV

300000 years atoms 15 Mrd years

  • ur Universe
slide-3
SLIDE 3

3 3

Heavy Heavy-

  • ion accelerators

ion accelerators

1 event: Au+Au, 21.3 TeV

  • Relativistic

Relativistic-

  • Heavy

Heavy-

  • Ion

Ion-

  • Collider

Collider – – RHIC RHIC -

  • (Brookhaven):

(Brookhaven): Au+Au at 21.3 A TeV Au+Au at 21.3 A TeV

  • Future facilities:

Future facilities: FAIR (GSI), NICA (Dubna) FAIR (GSI), NICA (Dubna)

  • Large

Large Hadron Collider Hadron Collider -

  • LHC

LHC -

  • (CERN):

(CERN): Pb+Pb at 574 A TeV Pb+Pb at 574 A TeV

L=3.8 km L=3.8 km

STAR detector at RHIC STAR detector at RHIC NICA NICA

SPS SPS L=27 km L=27 km

slide-4
SLIDE 4

4 4

0.5 1.0 1.5 2.0 2.5 3.0 2 4 6 8 10 12 14

  • Lattice QCD:

µ

µ µ µB=0

µ

µ µ µB=530 MeV

T/Tc

ε ε ε ε/T

4

The QGP in Lattice QCD The QGP in Lattice QCD

T Tc

c = 160 MeV

= 160 MeV

Lattice QCD: Lattice QCD:

energy density versus temperature energy density versus temperature Q Quantum uantum C Chromo hromo D Dynamics : ynamics : predicts strong increase of predicts strong increase of the the energy density energy density ε ε ε ε ε ε ε ε at a critical at a critical temperature temperature T TC

C ~160 MeV

~160 MeV ⇒ ⇒ Possible Possible phase transition phase transition from from hadronic to hadronic to partonic matter partonic matter (quarks, gluons) at critical energy (quarks, gluons) at critical energy density density ε ε ε ε ε ε ε εC

C ~0.5 GeV/fm

~0.5 GeV/fm3

3

Critical conditions Critical conditions -

  • ε

ε ε ε ε ε ε εC

C ~0.5 GeV/fm

~0.5 GeV/fm3

3 , T

, TC

C ~160 MeV

~160 MeV -

  • can be reached

can be reached in in heavy heavy-

  • ion experiments

ion experiments at bombarding energies at bombarding energies > 5 GeV/A > 5 GeV/A

QGP QGP

hadrons hadrons

slide-5
SLIDE 5

5 5

The holy grail of heavy The holy grail of heavy-

  • ion physics:

ion physics:

  • Study of the

Study of the phase phase transition transition from from hadronic to partonic hadronic to partonic matter matter – – Quark Quark-

  • Gluon

Gluon-

  • Plasma

Plasma

  • Search for the

Search for the critical point critical point

  • Study of the

Study of the in in-

  • medium

medium properties of hadrons at high baryon density properties of hadrons at high baryon density and temperature and temperature

The phase diagram of QCD The phase diagram of QCD

slide-6
SLIDE 6

6 6

‚Little Bangs‘ in the Laboratory

time

  • How can we prove that an equilibrium QGP has been

How can we prove that an equilibrium QGP has been created in central heavy created in central heavy-

  • ion collisions ?!

ion collisions ?!

PHSD PHSD

slide-7
SLIDE 7

7 7

  • Multi

Multi-

  • strange particle enhancement in A+A

strange particle enhancement in A+A

  • Charm suppression

Charm suppression

  • Collective flow (v

Collective flow (v1

1, v

, v2

2)

)

  • Thermal dileptons

Thermal dileptons

  • Jet quenching and angular correlations

Jet quenching and angular correlations

  • High p

High pT

T suppression of hadrons

suppression of hadrons

  • Nonstatistical event by event fluctuations and correlations

Nonstatistical event by event fluctuations and correlations

  • ...

...

Experiment: Experiment: measures

measures final hadrons and leptons final hadrons and leptons

Signals of the phase transition: Signals of the phase transition:

How to learn about How to learn about physics from data? physics from data? Compare with theory! Compare with theory!

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SLIDE 8

8 8

  • Statistical models:

Statistical models:

basic assumption basic assumption: system is described by a (grand) canonical ensemble of : system is described by a (grand) canonical ensemble of non non-

  • interacting fermions and bosons in

interacting fermions and bosons in thermal and chemical equilibrium thermal and chemical equilibrium [ [ -

  • :

: no dynamics]

no dynamics]

  • Ideal hydrodynamical models:

Ideal hydrodynamical models:

basic assumption basic assumption: conservation laws + equation of state; assumption of : conservation laws + equation of state; assumption of local thermal and chemical equilibrium local thermal and chemical equilibrium [ [ -

  • :

: -

  • simplified dynamics]

simplified dynamics]

  • Transport models:

Transport models:

based on transport theory of relativistic quantum many based on transport theory of relativistic quantum many-

  • body systems

body systems -

  • Actual solutions:

Actual solutions: Monte Carlo simulations Monte Carlo simulations [ [+:

+: full dynamics |

full dynamics | -

  • :

: very complicated]

very complicated]

Basic models for heavy Basic models for heavy-

  • ion collisions

ion collisions

  • Microscopic transport models provide a unique

Microscopic transport models provide a unique dynamical dynamical description description

  • f
  • f nonequilibrium

nonequilibrium effects in heavy effects in heavy-

  • ion collisions

ion collisions

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SLIDE 9

9 9

Semi Semi-

  • classical BUU equation

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

Boltzmann -

  • Uehling

Uehling-

  • Uhlenbeck equation

Uhlenbeck equation (non (non-

  • relativistic formulation)

relativistic formulation)

  • propagation of particles in the

propagation of particles in the self self-

  • generated Hartree

generated Hartree-

  • Fock mean

Fock mean-

  • field

field potential potential U(r,t) U(r,t) with an on with an on-

  • shell

shell collision term: 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

+ + + + ′ ′ ′ ′ ′ ′ ′ ′ − − − − ′ ′ ′ ′ = = = =

∑ ∑ ∑ ∑∫ ∫ ∫ ∫

  • β

β β β

π π π π

) t , p , r ( f

  • is the

is the single particle phase single particle phase-

  • space distribution function

space distribution function

  • probability to find the particle at position

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

  • self

self-

  • generated

generated Hartree Hartree-

  • Fock mean

Fock mean-

  • field potential:

field potential:

Ludwig Boltzmann

collision term: collision term: eleastic and eleastic and inelastic reactions 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

⋅ ⋅ ⋅ ⋅ + + + + → → → → + + + + ⋅ ⋅ ⋅ ⋅ − − − − − − − − + + + + = = = =

∫ ∫ ∫ ∫ ∫ ∫ ∫ ∫

Ω Ω Ω Ω σ σ σ σ δ δ δ δ υ υ υ υ Ω Ω Ω Ω π π π π

  • Probability including

Probability including Pauli blocking of fermions: 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 Gain term: 3+4

  • 1+2

1+2 Loss term: 1+2 Loss term: 1+2

  • 3+4

3+4 Collision term Collision term for 1+2 for 1+2

  • 3+4 (let

3+4 (let‘ ‘s consider fermions) s consider fermions) : : 1 2 3 4

t ∆ ∆ ∆ ∆

12

υ υ υ υ

slide-10
SLIDE 10

10 10

Dynamical description of strongly interacting systems Dynamical description of strongly interacting systems

  • Semi

Semi-

  • classical BUU

classical BUU

  • solution for weakly interacting systems of particles

solution for weakly interacting systems of particles How to describe How to describe strongly interacting systems?! strongly interacting systems?!

  • Quantum field theory

Quantum field theory

  • Kadanoff

Kadanoff-

  • Baym dynamics

Baym dynamics for resummed(!) single for resummed(!) single-

  • particle Green functions S

particle Green functions S<

<

(1962) (1962)

Leo Kadanoff Leo Kadanoff Gordon Baym Gordon Baym

) M ( S ˆ

2 x x 1 x

+ + + + ∂ ∂ ∂ ∂ ∂ ∂ ∂ ∂ − − − − ≡ ≡ ≡ ≡

− − − − µ µ µ µ µ µ µ µ

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 Green functions S<

< /self

/self-

  • energies

energies Σ: Σ: Σ: Σ: Σ: Σ: Σ: Σ:

  • perator
  • rdering

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

c a

− − − − − − − − − − − − ± ± ± ± = = = = η η η η

Integration over the intermediate spacetime Integration over the intermediate spacetime

slide-11
SLIDE 11

11 11

From Kadanoff From Kadanoff-

  • Baym equations to generalized

Baym equations to generalized transport equations transport equations

After the After the first order gradient expansion of the Wigner transformed first order gradient expansion of the Wigner transformed Kadanoff Kadanoff-

  • Baym equations

Baym equations and separation into the real and imaginary parts one gets: and separation into the real and imaginary parts one gets:

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

‚gain gain‘ ‘ term term backflow term backflow term

Generalized transport equations (GTE): Generalized transport equations (GTE):

Backflow term Backflow term incorporates the incorporates the off

  • ff-
  • shell

shell behavior in the particle propagation behavior in the particle propagation ! ! vanishes in the quasiparticle limit vanishes in the quasiparticle limit A AXP

XP

  • δ

δ δ δ δ δ δ δ(p (p2

2-

  • M

M2

2)

) Spectral function: Spectral function: – – width of spectral function width of spectral function = = reaction rate reaction rate of particle (at phase

  • f particle (at phase-
  • space position XP)

space position XP)

4 4-

  • dimentional generalizaton of the Poisson

dimentional generalizaton of the Poisson-

  • bracket:

bracket:

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

(2000) 445

  • GTE:

GTE: Propagation of the Green Propagation of the Green‘ ‘s function s function i iS S<

<XP XP=A

=AXP

XPN

NXP

XP , which carries information not

, which carries information not

  • nly on the
  • nly on the number of particles

number of particles ( (N NXP

XP)

), but also on their , but also on their properties, properties, interactions and interactions and correlations correlations (via (via A AXP

XP)

)

ret XP XP

ImΣ Σ Σ Σ Γ Γ Γ Γ − − − − = = = =

slide-12
SLIDE 12

12 12

HSD HSD – – H Hadron adron-

  • S

String tring-

  • D

Dynamics transport approach: ynamics transport approach:

  • solution of

solution of the the generalized off generalized off-

  • shell transport equations

shell transport equations for for the phase the phase-

  • space density

space density f fi

i(r,p,t)

(r,p,t) with with collision terms collision terms I Icoll

coll describing:

describing:

The baseline concepts of HSD The baseline concepts of HSD

HSD is an open code: HSD is an open code: http://www.th.physik.uni-frankfurt.de/~brat/hsd.html

Low energy collisions: Low energy collisions:

  • binary 2

binary 2< < < < < < < <− − − − − − − −>2 >2 >2 >2 >2 >2 >2 >2 and and 2 2< < < < < < < <− − − − − − − −> > > > > > > >3 reactions 3 reactions

  • 1

1< < < < < < < <− − − − − − − −>2 >2 >2 >2 >2 >2 >2 >2 : formation and : formation and decay of baryonic and decay of baryonic and mesonic mesonic resonances resonances BB BB < < < < < < < <− − − − − − − −> > > > > > > > B´B´ B´B´ BB BB < < < < < < < <− − − − − − − −> > > > > > > > B´B´m B´B´m mB mB < < < < < < < <− − − − − − − −> > > > > > > > m´B´ m´B´ mB mB < < < < < < < <− − − − − − − −> > > > > > > > B´ B´ mm mm < < < < < < < <− − − − − − − −> > > > > > > > m´m´ m´m´ mm mm < < < < < < < <− − − − − − − −> > > > > > > > m´ m´ . . . . . . Baryons: Baryons: B = p, n, B = p, n, ∆(1232) ∆(1232) ∆(1232) ∆(1232) ∆(1232) ∆(1232) ∆(1232) ∆(1232), , N(1440), N(1535), ... N(1440), N(1535), ... Mesons: Mesons: M = M = π π π π π π π π, , η η η η η η η η, , ρ, ω, φ, ... ρ, ω, φ, ... ρ, ω, φ, ... ρ, ω, φ, ... ρ, ω, φ, ... ρ, ω, φ, ... ρ, ω, φ, ... ρ, ω, φ, ...

π π π π π π π π+

+p

p pp pp

High energy collisions: High energy collisions: (above s (above s1/2

1/2~2.5 GeV)

~2.5 GeV) Inclusive particle Inclusive particle production: production: BB BB − − − − − − − −> > > > > > > > X , mB X , mB − − − − − − − −> > > > > > > >X X X =many particles X =many particles described by described by strings strings (= excited color (= excited color singlet states singlet states q q-

  • qq

qq, , q q-

  • qbar

qbar) ) formation and decay formation and decay

slide-13
SLIDE 13

13 13

  • very good description of particle production in

very good description of particle production in pp, pA, pp, pA, π π π π π π π πA, AA reactions A, AA reactions

  • unique description of nuclear dynamics

unique description of nuclear dynamics from from low low (~100 MeV) (~100 MeV) to ultrarelativistic to ultrarelativistic (>20 TeV) energies (>20 TeV) energies

HSD HSD – – a microscopic off a microscopic off-

  • shell transport model

shell transport model for heavy for heavy-

  • ion reactions

ion reactions

10

  • 1

10 10

1

10

2

10

3

10

4

10

  • 6

10

  • 4

10

  • 2

10 10

2

10

4

AGS SPS RHIC

HSD ' 99

__ D(c) J/Ψ

Ψ Ψ Ψ

D(c)

φ φ φ φ

K

− − − −

K

+

η η η η π π π π

+

Multiplicity

Au+Au (central)

Energy [A GeV]

HSD predictions from 1999; data from the new millenium HSD predictions from 1999; data from the new millenium

slide-14
SLIDE 14

14 14

Hadron Hadron-

  • string

string transport models (HSD, UrQMD) transport models (HSD, UrQMD) versus observables versus observables

10 10

1

10

2

10

3

10

4

0.00 0.05 0.10 0.15 0.20 0.25

E866 NA49 BRAHMS, 5%

HSD UrQMD

<K

+>/<π

π π π

+>

Elab/A [GeV] 1 10 100 0.10 0.15 0.20 0.25 0.30 0.35

s

1/2 [GeV]

E866 NA49 NA44 STAR BRAHMS PHENIX

Au+Au / Pb+Pb -> K

++X

T [GeV]

HSD HSD with Cronin eff. UrQMD

‚horn horn‘ ‘ in K in K+

+/

/π π π π π π π π+

+

‚step step‘ ‘ in slope T in slope T

  • Exp. data are not reproduced in terms
  • Exp. data are not reproduced in terms
  • f the hadron
  • f the hadron-
  • string picture

string picture => evidence for => evidence for partonic degrees of partonic degrees of freedom freedom

PRC 69 (2004) 032302 PRC 69 (2004) 032302

  • elliptic flow

elliptic flow

slide-15
SLIDE 15

15 15

Goal: Goal: microscopic transport description of microscopic transport description of the the partonic partonic and and hadronic phase hadronic phase

Problems: Problems:

  • How to model a

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

  • How to solve the

How to solve the hadronization problem hadronization problem? ?

Ways to go: Ways to go:

‚ ‚Hybrid

Hybrid‘ ‘ models: models:

  • QGP phase:

QGP phase: hydro hydro with QGP EoS with QGP EoS

  • hadronic freeze

hadronic freeze-

  • out: after burner
  • ut: after burner
  • hadron

hadron-

  • string transport model

string transport model

  • Hybrid

Hybrid-

  • UrQMD

UrQMD

  • microscopic

microscopic transport description of the transport description of the partonic partonic and and hadronic phase hadronic phase in terms of strongly interacting in terms of strongly interacting dynamical dynamical quasi quasi-

  • particles

particles and off and off-

  • shell hadrons

shell hadrons

  • PHSD

PHSD pQCD based models: pQCD based models:

  • QGP phase: pQCD cascade

QGP phase: pQCD cascade

  • hadronization: quark coalescence

hadronization: quark coalescence

  • AMPT, HIJING, BAMPS

AMPT, HIJING, BAMPS

slide-16
SLIDE 16

16 16

From hadrons to partons From hadrons to partons

In order to study the In order to study the phase transition phase transition from from hadronic to partonic matter hadronic to partonic matter – – Quark Quark-

  • Gluon

Gluon-

  • Plasma

Plasma – – we we need need a a consistent non consistent non-

  • equilibrium (transport) model with

equilibrium (transport) model with

  • explicit

explicit parton parton-

  • parton interactions

parton interactions (i.e. between quarks and gluons) (i.e. between quarks and gluons) beyond strings! beyond strings!

  • explicit

explicit phase transition phase transition from hadronic to partonic degrees of freedom from hadronic to partonic degrees of freedom

  • lQCD EoS

lQCD EoS for partonic phase for partonic phase

P Parton arton-

  • H

Hadron adron-

  • S

String tring-

  • D

Dynamics ( ynamics (PHSD PHSD) )

QGP phase QGP phase described by described by D Dynamical ynamical Q Quasi uasiP Particle article M Model

  • del (DQPM

DQPM) Transport theory Transport theory: off : off-

  • shell Kadanoff

shell Kadanoff-

  • Baym equations for the

Baym equations for the Green Green-

  • functions S

functions S<

< h h(x,p) in phase

(x,p) in phase-

  • space representation for the

space representation for the partonic partonic and and hadronic phase hadronic phase

A.

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

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

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

NPA831 (2009) 215; NPA831 (2009) 215;

  • W. Cassing,
  • W. Cassing, E

EPJ ST PJ ST 168 168 (2009) (2009) 3 3

slide-17
SLIDE 17

17 17

DQPM DQPM describes describes QCD QCD properties in terms of properties in terms of ‚ ‚resummed resummed‘ ‘ single single-

  • particle Green

particle Green‘ ‘s s functions functions – – in the sense of a two in the sense of a two-

  • particle irreducible (

particle irreducible (2PI 2PI) approach: ) approach:

A.

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

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

Dynamical QuasiParticle Model (DQPM) Dynamical QuasiParticle Model (DQPM) -

  • Basic ideas:

Basic ideas:

  • the

the resummed resummed properties are specified by properties are specified by complex self complex self-

  • energies

energies which depend on which depend on temperature temperature: :

  • - the

the real part of self real part of self-

  • energies

energies ( (Σ Σq

q,

, Π Π) ) describes a describes a dynamically generated dynamically generated mass mass ( (M Mq

q,M

,Mg

g)

); ;

  • - the

the imaginary part imaginary part describes the describes the interaction width interaction width of

  • f partons

partons ( (Γ Γ Γ Γ Γ Γ Γ Γq

q,

, Γ Γ Γ Γ Γ Γ Γ Γg

g)

)

  • space

space-

  • like part of energy

like part of energy-

  • momentum tensor

momentum tensor T Tµν

µν µν µν µν µν µν µν defines the potential energy

defines the potential energy density and the density and the mean mean-

  • field potential

field potential (1PI) for quarks and gluons (1PI) for quarks and gluons

  • 2PI frame

2PI framew work

  • rk guarant

guaranti ies es a consistent description of the system a consistent description of the system in in-

  • and out

and out-

  • of
  • f

equilibrium equilibrium on the basis of

  • n the basis of Kadanoff

Kadanoff-

  • Baym

Baym equations equations

Gluon propagator: Gluon propagator:

  • 1

1 =P

=P2

2 -

  • Π

Π gluon self gluon self-

  • energy:

energy: Π Π=M =Mg

g2 2-

  • i2

i2Γ Γ Γ Γ Γ Γ Γ Γg

ω Quark propagator: Quark propagator: S Sq

q

  • 1

1 = P

= P2

2 -

  • Σ

Σq

q

quark self quark self-

  • energy:

energy: Σ Σq

q=M

=Mq

q2 2-

  • i2

i2Γ Γ Γ Γ Γ Γ Γ Γq

ω

slide-18
SLIDE 18

18 18

The Dynamical QuasiParticle Model (DQPM) The Dynamical QuasiParticle Model (DQPM)

Properties Properties of

  • f interacting quasi

interacting quasi-

  • particles:

particles: massive quarks and gluons massive quarks and gluons (g, q, q (g, q, qbar

bar)

) with with Lorentzian spectral functions : Lorentzian spectral functions :

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

with with 3 parameters: 3 parameters: T Ts

s/T

/Tc

c=0.46;

=0.46; c c=28.8; =28.8; λ λ λ λ λ λ λ λ=2.42 =2.42

(for pure glue N (for pure glue Nf

f=0)

=0)

  • fit to lattice (lQCD) results

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

( ( ( ( ) ) ) )

(T) ω 4 (T) M p ω (T) ω 4 ) T , ( ρ

2 i 2 2 2 i 2 2 i i

Γ Γ Γ Γ Γ Γ Γ Γ ω ω ω ω + + + + − − − − − − − − = = = =

  • )

g , q , q i ( = = = =

  • running coupling

running coupling (pure glue): (pure glue):

N Nc

c = 3, N

= 3, Nf

f=3

=3

mass: mass: width: width:

  • gluons:

gluons:

  • quarks:

quarks:

lQCD: pure glue lQCD: pure glue

  • Modeling of the quark/gluon masses and widths

Modeling of the quark/gluon masses and widths

  • HTL limit at high T

HTL limit at high T

slide-19
SLIDE 19

19 19

The Dynamical QuasiParticle Model (DQPM) The Dynamical QuasiParticle Model (DQPM)

Peshier, Cassing, PRL 94 (2005) 172301; Cassing, NPA 791 (2 Peshier, Cassing, PRL 94 (2005) 172301; Cassing, NPA 791 (2007) 365: NPA 793 (2007) 007) 365: NPA 793 (2007)

  • Quasiparticle properties:

Quasiparticle properties:

  • large width and mass for gluons and quarks

large width and mass for gluons and quarks

  • DQPM

DQPM matches well matches well lattice QCD lattice QCD

  • DQPM

DQPM provides provides mean mean-

  • fields (1PI) for gluons and quarks

fields (1PI) for gluons and quarks as well as as well as effective 2 effective 2-

  • body interactions (2PI)

body interactions (2PI)

  • DQPM

DQPM gives gives transition rates transition rates for the formation of hadrons for the formation of hadrons

  • PHSD

PHSD

  • fit to lattice (lQCD) results

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

(e.g. entropy density)

* BMW lQCD data S. Borsanyi et al., JHEP 1009 (2010) 073 * BMW lQCD data S. Borsanyi et al., JHEP 1009 (2010) 073 Plot from Peshier, Plot from Peshier, PRD 70 (2004) PRD 70 (2004) 034016 034016

T TC

C=158 MeV

=158 MeV ε ε ε ε ε ε ε εC

C=0.5 GeV/fm

=0.5 GeV/fm3

3

slide-20
SLIDE 20

20 20

  • Formation of QGP stage

Formation of QGP stage by dissolution of pre by dissolution of pre-

  • hadrons

hadrons (all new produced secondary hadrons) (all new produced secondary hadrons) into into massive colored quarks + mean massive colored quarks + mean-

  • field energy

field energy based on the based on the Dynamical Quasi Dynamical Quasi-

  • Particle Model (DQPM)

Particle Model (DQPM) which defines which defines quark spectral functions, quark spectral functions, i.e. masses i.e. masses M Mq

q(

(ε ε ε ε ε ε ε ε) ) and widths and widths Γ Γ Γ Γ Γ Γ Γ Γq

q (

(ε ε ε ε ε ε ε ε) ) + + mean mean-

  • field potential

field potential U Uq

q at given

at given ε ε ε ε ε ε ε ε – – local energy density local energy density

( (ε ε ε ε ε ε ε ε related by lQCD EoS to related by lQCD EoS to T T -

  • temperature in the local cell)

temperature in the local cell)

  • I. PHSD
  • I. PHSD -
  • basic concept

basic concept

  • Initial A+A collisions

Initial A+A collisions – – as in HSD: as in HSD:

  • string

string formation in primary NN collisions formation in primary NN collisions

  • string decay to

string decay to pre pre-

  • hadrons

hadrons ( (B B -

  • baryons,

baryons, m m -

  • mesons)

mesons)

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

NPA831 (2009) 215; NPA831 (2009) 215; E EPJ ST PJ ST 168 168 (2009) (2009) 3 3; ; N NP PA856 A856 (2011) (2011) 162 162. .

QGP phase: QGP phase: ε ε ε ε ε ε ε ε > > ε ε ε ε ε ε ε εcritical

critical

q

U q q m qqq, B ∀ ∀ ∀ ∀ → → → → → → → →

I.

  • I. From hadrons to QGP:

From hadrons to QGP:

slide-21
SLIDE 21

21 21

  • II. PHSD
  • II. PHSD -
  • basic concept

basic concept

g g g g g q q + + + + → → → → + + + + → → → → + + + +

II.

  • II. Partonic phase

Partonic phase -

  • QGP:

QGP:

quarks and gluons (= quarks and gluons (= ‚ ‚dynamical quasiparticles dynamical quasiparticles‘ ‘) ) with with off

  • ff-
  • shell spectral functions

shell spectral functions (width, mass) defined by the DQPM (width, mass) defined by the DQPM

  • in

in self self-

  • generated mean

generated mean-

  • field potential

field potential for quarks and gluons for quarks and gluons U Uq

q, U

, Ug

g

from the DQPM from the DQPM

  • EoS of partonic phase:

EoS of partonic phase: ‚crossover‘ from lattice QCD ‚crossover‘ from lattice QCD (fitted by DQPM) (fitted by DQPM)

  • (quasi

(quasi-

  • ) elastic and inelastic

) elastic and inelastic parton parton-

  • parton interactions:

parton interactions: using the effective cross sections from the DQPM using the effective cross sections from the DQPM

  • (quasi

(quasi-

  • ) elastic collisions:

) elastic collisions:

  • inelastic collisions:

inelastic collisions: (Breit (Breit-

  • Wigner cross sections)

Wigner cross sections)

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 + + + + → → → → + + + + + + + + → → → → + + + + + + + + → → → → + + + +

suppressed (<1%) suppressed (<1%) due to the large due to the large mass of gluons mass of gluons

slide-22
SLIDE 22

22 22

  • III. PHSD
  • III. PHSD -
  • basic concept

basic concept

III.

  • III. Hadronization:

Hadronization:

  • Hadronization:

Hadronization: based on DQPM based on DQPM

  • massive, off

massive, off-

  • shell (anti

shell (anti-

  • )quarks

)quarks with broad spectral functions hadronize to with broad spectral functions hadronize to

  • ff
  • ff-
  • shell mesons and baryons or color neutral excited states

shell mesons and baryons or color neutral excited states -

‚strings strings‘ ‘ (strings act as (strings act as ‚ ‚doorway states doorway states‘ ‘ for hadrons) for hadrons)

) ' string (' baryon q q q ) ' string (' meson q q , q q g ↔ ↔ ↔ ↔ + + + + + + + + ↔ ↔ ↔ ↔ + + + + + + + + → → → →

IV.

  • IV. Hadronic phase:

Hadronic phase: hadron

hadron-

  • string interactions

string interactions – – off

  • ff-
  • shell HSD

shell HSD

  • Local covariant off

Local covariant off-

  • shell

shell transition rate transition rate for q+qbar fusion for q+qbar fusion

  • meson formation:

meson formation:

  • N

Nj

j(x,p)

(x,p) is the phase is the phase-

  • space density of parton j at space

space density of parton j at space-

  • time position

time position x x and 4 and 4-

  • momentum

momentum p p

  • W

Wm

m is the phase

is the phase-

  • space distribution of the formed

space distribution of the formed ‚ ‚pre pre-

  • hadrons

hadrons‘ ‘ (Gaussian in phase space) (Gaussian in phase space)

|Μ |Μ |Μ |Μ |Μ |Μ |Μqq

qq|

| | | | | | |2

2 2 2 2 2 2 2 is the effective quark

is the effective quark-

  • antiquark interaction from the DQPM

antiquark interaction from the DQPM

( ( ( ( ) ) ) )

q q q q m 2 q q q q q q q q q q q q q q q q 4 q q 4 q q 4 4 m q q

p p , x x W | M | ) p ( ) p ( ) p , x ( N ) p , x ( N ) color , flavor ( x 2 x x ) p p p ( Tr Tr p d x d dN − − − − − − − − ⋅ ⋅ ⋅ ⋅ ⋅ ⋅ ⋅ ⋅ ⋅ ⋅ ⋅ ⋅ ⋅ ⋅ ⋅ ⋅                                 − − − − + + + + − − − − − − − − = = = =

→ → → → + + + +

ρ ρ ρ ρ ω ω ω ω ρ ρ ρ ρ ω ω ω ω δ δ δ δ δ δ δ δ δ δ δ δ

slide-23
SLIDE 23

23 23

PHSD PHSD – – ‚ ‚femto femto‘ ‘ accelerator accelerator

slide-24
SLIDE 24

24 24

Au+Au, 21.3 TeV, central Au+Au, 21.3 TeV, central

slide-25
SLIDE 25

25 25

Properties of QGP Properties of QGP in in-

  • equilibrium

equilibrium using PHSD using PHSD

slide-26
SLIDE 26

26 26

The goal: The goal:

  • study of the

study of the dynamical equilibration dynamical equilibration of QGP within the non

  • f QGP within the non-
  • equilibrium

equilibrium

  • ff
  • ff-
  • shell

shell PHSD PHSD transport approach transport approach

  • transport coefficients

transport coefficients (shear and bulk viscosities) (shear and bulk viscosities) of

  • f strongly

strongly interacting interacting partonic partonic matter matter

  • particle number

particle number fluctuations fluctuations (scaled variance, skewness, (scaled variance, skewness, kurtosis) kurtosis)

Properties of parton Properties of parton-

  • hadron matter in

hadron matter in-

  • equlibrium

equlibrium

  • V. Ozvenchuk et al., PRC 87 (2013)
  • V. Ozvenchuk et al., PRC 87 (2013) 064903

064903, , arXiv:1212.5393 arXiv:1212.5393

Realization: Realization:

  • Initialize the system in a

Initialize the system in a finite box with finite box with periodic boundary conditions periodic boundary conditions with some with some energy density energy density ε ε and chemical potential and chemical potential q

q

  • Evolve the system in time

Evolve the system in time until until equilibrium is achieved equilibrium is achieved

  • V. Ozvenchuk et al., PRC 87 (2013) 024901, arXiv:1203.4734
  • V. Ozvenchuk et al., PRC 87 (2013) 024901, arXiv:1203.4734
slide-27
SLIDE 27

27 27

Properties of parton Properties of parton-

  • hadron matter

hadron matter – – shear viscosity shear viscosity

T=T

T=TC

C:

: η η η η η η η η/s /s shows shows a a minimum minimum (~0.1) (~0.1) close to the critical temperature close to the critical temperature

  • T>T

T>TC

C :

: QGP QGP -

  • pQCD

pQCD limit limit at higher at higher temperatures temperatures

  • T<T

T<TC

C:

: fast increase of the ratio fast increase of the ratio η η η η η η η η/s /s for for hadronic matter hadronic matter

  • lower interaction rate of hadronic

lower interaction rate of hadronic system system

  • smaller number of degrees of freedom

smaller number of degrees of freedom (or entropy density) (or entropy density) for hadronic for hadronic matter compared to the QGP matter compared to the QGP

QGP QGP in PHSD in PHSD = = strongly strongly-

  • interacting liquid

interacting liquid

η η η η η η η η/s /s using using Kubo formalism Kubo formalism and the and the relaxation time approximation relaxation time approximation (‚kinetic theory‘) (‚kinetic theory‘)

Virial expansion: Virial expansion: S.

  • S. Mattiello

Mattiello, , W.

  • W. Cassing

Cassing, , Eur

  • Eur. Phys. J. C 70, 243

. Phys. J. C 70, 243 (2010). (2010).

  • V. Ozvenchuk et al., PRC 87 (2013)
  • V. Ozvenchuk et al., PRC 87 (2013) 064903

064903

QGP QGP

slide-28
SLIDE 28

28 28

Properties of parton Properties of parton-

  • hadron matter

hadron matter – – electric conductivity electric conductivity

  • the

the QCD QCD matter matter even at T even at T~ ~ T Tc

c is a

is a much better much better electric conductor than Cu or Ag electric conductor than Cu or Ag (at room (at room temperature temperature) ) by a factor of 500 ! by a factor of 500 !

  • The response of the strongly

The response of the strongly-

  • interacting

interacting system in equilibrium to an system in equilibrium to an external electric external electric field field eE eEz

z defines the

defines the electric conductivity electric conductivity σ σ σ σ σ σ σ σ0

0:

:

  • W. Cassing et al., PRL 110(2013)182301
  • W. Cassing et al., PRL 110(2013)182301
slide-29
SLIDE 29

29 29

Bulk properties: Bulk properties: rapidity, m rapidity, mT

T-

  • distributions,

distributions, multi multi-

  • strange particle enhancement in Au+Au

strange particle enhancement in Au+Au

slide-30
SLIDE 30

30 30

PHSD: Transverse mass spectra PHSD: Transverse mass spectra

Central Pb + Pb at SPS energies Central Pb + Pb at SPS energies

  • PHSD gives

PHSD gives harder m harder mT

T spectra

spectra and works better than HSD and works better than HSD at high energies at high energies – – RHIC, SPS (and top FAIR, NICA) RHIC, SPS (and top FAIR, NICA)

  • however, at low SPS (and low FAIR, NICA) energies the effect of

however, at low SPS (and low FAIR, NICA) energies the effect of the partonic phase the partonic phase decreases due to the decrease of the partonic fraction decreases due to the decrease of the partonic fraction Central Au+Au at RHIC Central Au+Au at RHIC

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

NPA856 (2011) 162 NPA856 (2011) 162

slide-31
SLIDE 31

31 31

Centrality dependence of (multi Centrality dependence of (multi-

  • )strange (anti

)strange (anti-

  • )baryons

)baryons

  • enhanced production of (multi

enhanced production of (multi-

  • ) strange antibaryons in PHSD

) strange antibaryons in PHSD relative to HSD relative to HSD strange strange antibaryons antibaryons _ _ _ _ Λ Λ Λ Λ Λ Λ Λ Λ+ +Σ Σ Σ Σ Σ Σ Σ Σ0 multi multi-

  • strange

strange antibaryon antibaryon _ _ Ξ Ξ Ξ Ξ Ξ Ξ Ξ Ξ+

+

100 200 300 400 0.00 0.01 0.02 0.03 0.04 0.05 0.06 100 200 300 400 0.000 0.002 0.004 0.006 0.008 0.010

NA57 NA49 HSD PHSD

Λ

Λ Λ Λ+Σ Σ Σ Σ

Nwound Nwound

Pb+Pb, 158 A GeV, mid-rapidity

_ _ Λ+Σ

Λ+Σ Λ+Σ Λ+Σ

dN/dy | y=0 / Nwound

100 200 300 400 10

  • 4

10

  • 3

10

  • 2

100 200 300 400 10

  • 4

10

  • 3

HSD PHSD NA57 NA49

Ξ

Ξ Ξ Ξ

− − − −

dN/dy | y=0 / Nwound

__ __ __ __

Ξ

Ξ Ξ Ξ

+ + + +

Pb+Pb, 158 A GeV, mid-rapidity

Nwound Nwound

multi multi-

  • strange

strange baryon baryon Ξ Ξ Ξ Ξ Ξ Ξ Ξ Ξ

− − − − − − − −-

  • strange

strange baryons baryons Λ Λ Λ Λ Λ Λ Λ Λ+ +Σ Σ Σ Σ Σ Σ Σ Σ0

Cassing & Bratkovskaya, NPA 831 (2009) 215 Cassing & Bratkovskaya, NPA 831 (2009) 215

slide-32
SLIDE 32

32 32

Collective flow: Collective flow: anisotropy coefficients (v anisotropy coefficients (v1

1, v

, v2,

2, v

v3

3, , v

v4

4)

) in A+A in A+A

x z

slide-33
SLIDE 33

33 33

Anisotropy coefficients Anisotropy coefficients

Non central Non central Au+Au Au+Au collisions : collisions :

  • i

interaction nteraction between constituents between constituents leads to a leads to a pressure pressure gradient gradient => spatial asymmetry => spatial asymmetry is is converted converted to to an an asymmetry in momentum space asymmetry in momentum space => => collective flow collective flow v v2

2 > 0

> 0 indicates indicates in in-

  • plane

plane emission of particles emission of particles v v2

2 < 0

< 0 corresponds to a corresponds to a squeeze squeeze-

  • out
  • ut perpendicular

perpendicular to the reaction plane ( to the reaction plane (out

  • ut-
  • of
  • f-
  • plane

plane emission) emission) v v2

2 > 0

> 0

from S. A. Voloshin, arXiv:1111.7241 from S. A. Voloshin, arXiv:1111.7241

slide-34
SLIDE 34

34 34

Development of azimuthal anisotropies in time Development of azimuthal anisotropies in time

Flow coefficients

Flow coefficients reach their asymptotic values reach their asymptotic values by the time of 6 by the time of 6– –8 fm 8 fm/c /c after after the beginning of the collision the beginning of the collision

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

Time evolution of Time evolution of v vn

n for Au + Au collisions at

for Au + Au collisions at s s 1/2

1/2 = 200 GeV with impact

= 200 GeV with impact parameter parameter b b = 8 fm. = 8 fm.

slide-35
SLIDE 35

35 35

Elliptic flow v Elliptic flow v2

2 vs. collision energy for Au+Au

  • vs. collision energy for Au+Au

v

v2

2 in PHSD is larger than in HSD

in PHSD is larger than in HSD due to due to the repulsive scalar mean the repulsive scalar mean-

  • field potential

field potential U Us

s(

(ρ ρ) for partons ) for partons

  • v

v2

2 grows with bombarding energy

grows with bombarding energy due to due to the increase of the parton fraction the increase of the parton fraction

  • V. Konchakovski, E. Bratkovskaya, W. Cassing, V. Toneev, V. V
  • V. Konchakovski, E. Bratkovskaya, W. Cassing, V. Toneev, V. Voronyuk,
  • ronyuk,
  • Phys. Rev. C 85 (2012) 011902
  • Phys. Rev. C 85 (2012) 011902
slide-36
SLIDE 36

36 36

Scaling properties: quark number scaling Scaling properties: quark number scaling

The mass splitting at low p

The mass splitting at low pT

T is approximately reproduced as well as the

is approximately reproduced as well as the meson meson-

  • baryon splitting for p

baryon splitting for pT

T > 2 GeV/c !

> 2 GeV/c !

  • The

The scaling of v scaling of v2

2 with the number of constituent quarks n

with the number of constituent quarks nq

q is roughly in

is roughly in line with the data at RHIC. line with the data at RHIC.

  • E. Bratkovskaya, W. Cassing, V. Konchakovski, O. Linnyk,
  • E. Bratkovskaya, W. Cassing, V. Konchakovski, O. Linnyk,

NPA856 (2011) 162 NPA856 (2011) 162

slide-37
SLIDE 37

37 37

Dileptons Dileptons

slide-38
SLIDE 38

38 38

Electromagnetic probes: dileptons and photons Electromagnetic probes: dileptons and photons

iessen Joachim Stroth

Dilepton sources: Dilepton sources:

  • from the QGP via partonic (q,qbar, g) interactions:

from the QGP via partonic (q,qbar, g) interactions:

  • from hadronic sources:

from hadronic sources:

  • direct decay of vector

direct decay of vector mesons ( mesons (ρ,ω,φ, ρ,ω,φ, ρ,ω,φ, ρ,ω,φ, ρ,ω,φ, ρ,ω,φ, ρ,ω,φ, ρ,ω,φ,J J/Ψ,Ψ /Ψ,Ψ /Ψ,Ψ /Ψ,Ψ /Ψ,Ψ /Ψ,Ψ /Ψ,Ψ /Ψ,Ψ‘ ‘) )

  • Dalitz decay of mesons

Dalitz decay of mesons and baryons ( and baryons (π π π π π π π π0

0,

,η η η η η η η η, , ∆ ∆ ∆ ∆ ∆ ∆ ∆ ∆, ,… …) )

  • correlated D+Dbar pairs

correlated D+Dbar pairs

  • radiation from multi

radiation from multi-

  • meson reactions (

meson reactions (π π π π π π π π+ +π π π π π π π π, , π π π π π π π π+ +ρ ρ ρ ρ ρ ρ ρ ρ, , π π π π π π π π+ +ω ω ω ω ω ω ω ω, , ρ ρ ρ ρ ρ ρ ρ ρ+ +ρ ρ ρ ρ ρ ρ ρ ρ , , π π π π π π π π+a +a1

1)

) -

‚4 4π π π π π π π π‘ ‘

  • Dileptons are

Dileptons are an ideal probe an ideal probe to study the to study the properties of the hot and dense medium properties of the hot and dense medium

γ γ γ γ γ γ γ γ* * g g γ γ γ γ γ γ γ γ* * γ γ γ γ γ γ γ γ* * q q l+ l-

  • γ

γ γ γ γ γ γ γ*

*

q q q q q q q q q q q q g g g g q q

  • Dileptons are emitted from different stages of the reaction and

Dileptons are emitted from different stages of the reaction and not much effected by final not much effected by final-

  • state interactions

state interactions

slide-39
SLIDE 39

39 39

Dileptons Dileptons at SPS: NA60 at SPS: NA60

  • Mass region above 1

Mass region above 1 GeV GeV is dominated is dominated by by partonic partonic radiation radiation ! ! Acceptance corrected NA60 data Acceptance corrected NA60 data

  • O. Linnyk, E.B., V. Ozvenchuk, W. Cassing
  • O. Linnyk, E.B., V. Ozvenchuk, W. Cassing

and C. and C.-

  • M. Ko, PRC 84 (2011)
  • M. Ko, PRC 84 (2011) 054917

054917

  • Contributions of

Contributions of “ “4 4π π π π π π π π” ” channels channels ( (radiation from multi radiation from multi-

  • meson reactions)

meson reactions) are are small small

slide-40
SLIDE 40

40 40

NA60: m NA60: mT

T spectra

spectra

  • Inverse slope parameter T

Inverse slope parameter Teff

eff for

for dilepton spectra vs NA60 data dilepton spectra vs NA60 data Conjecture: Conjecture:

  • spectrum from sQGP is softer than from hadronic phase

spectrum from sQGP is softer than from hadronic phase since quark since quark-

  • antiquark

antiquark annihilation occurs dominantly before the collective radial flow annihilation occurs dominantly before the collective radial flow has developed (cf. has developed (cf. NA60) NA60)

  • O. Linnyk, E.B., V. Ozvenchuk, W. Cassing
  • O. Linnyk, E.B., V. Ozvenchuk, W. Cassing

and C. and C.-

  • M. Ko, PRC 84 (2011)
  • M. Ko, PRC 84 (2011) 054917

054917

slide-41
SLIDE 41

41 41

STAR: mass spectra STAR: mass spectra

  • O. Linnyk, W. Cassing, J. Manninen, E.B. and C.
  • O. Linnyk, W. Cassing, J. Manninen, E.B. and C.-
  • M. Ko, PRC 85 (2012) 024910
  • M. Ko, PRC 85 (2012) 024910
  • The

The partonic partonic channels channels dominate at M>1 dominate at M>1 GeV GeV

slide-42
SLIDE 42

42 42

LHC: mass spectra with exp. cuts LHC: mass spectra with exp. cuts

  • p

pT

T cut enhances the signal of

cut enhances the signal of QGP( QGP(qbar qbar-

  • q)

q)

  • O. Linnyk, W. Cassing, J. Manninen, E.B., P.B. Gossiaux, J. Aic
  • O. Linnyk, W. Cassing, J. Manninen, E.B., P.B. Gossiaux, J. Aichelin,

helin,

  • T. Song, C.
  • T. Song, C.-
  • M. Ko,
  • M. Ko, Phys.Rev. C87 (2013) 014905

Phys.Rev. C87 (2013) 014905; arXiv:1208.1279 ; arXiv:1208.1279

  • QGP(

QGP(qbar qbar-

  • q)

q) dominates at M>1.2 dominates at M>1.2 GeV GeV ! ! D D-

  • , B

, B-

  • mesons:

mesons: from from Pol Pol-

  • Bernard

Bernard Gossiaux Gossiaux and and J Jö örg Aichelin rg Aichelin J/ J/Ψ, Ψ Ψ, Ψ Ψ, Ψ Ψ, Ψ Ψ, Ψ Ψ, Ψ Ψ, Ψ Ψ, Ψ’ ’: : from C.M. from C.M. Ko Ko and T. Song and T. Song

slide-43
SLIDE 43

43 43

Summary Summary

  • PHSD

PHSD provides a consistent description of provides a consistent description of off

  • ff-
  • shell parton dynamics

shell parton dynamics in line with the lattice QCD equation of state in line with the lattice QCD equation of state (from the BMW (from the BMW collaboration) collaboration)

  • PHSD versus

PHSD versus experimental observables experimental observables: : enhancement of meson m enhancement of meson mT

T slopes (at top SPS and RHIC)

slopes (at top SPS and RHIC) strange antibaryon enhancement (at SPS) strange antibaryon enhancement (at SPS) partonic emission of high mass dileptons at SPS and RHIC partonic emission of high mass dileptons at SPS and RHIC enhancement of collective flow v enhancement of collective flow v2

2 with increasing energy

with increasing energy quark number scaling of v quark number scaling of v2

2 (at RHIC)

(at RHIC) … …

⇒ ⇒ evidence for strong nonhadronic interactions in the evidence for strong nonhadronic interactions in the early phase of relativistic heavy early phase of relativistic heavy-

  • ion reactions

ion reactions ⇒ ⇒ formation of the sQGP! formation of the sQGP!

slide-44
SLIDE 44

44 44

Outlook Outlook -

  • Perspectives

Perspectives

What is the stage of matter close to T What is the stage of matter close to Tc

c :

:

  • 1st order phase transition?

1st order phase transition?

‚Mixed Mixed‘ ‘ phase = interaction of partonic phase = interaction of partonic and hadronic degrees of freedom? and hadronic degrees of freedom?

(V.D. Toneev et al.) (V.D. Toneev et al.)

Open problems: Open problems:

  • How to describe a

How to describe a first first-

  • order phase
  • rder phase

transition transition in transport models? in transport models?

  • How to describe parton

How to describe parton-

  • hadron interactions in

hadron interactions in a ‚mixed‘ phase a ‚mixed‘ phase? ?

Lattice EQS for Lattice EQS for µ µ µ µ µ µ µ µ=0 =0

  • ‚crossover‘ , T > T

‚crossover‘ , T > Tc

c

slide-45
SLIDE 45

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HIC experiments HIC experiments

Baryonic matter Baryonic matter || || Meson and baryon Meson and baryon spectroscopy spectroscopy In In-

  • medium effects

medium effects EoS EoS

0.1 1 10 100 1000 10000 100000

Low Low Intermediate Intermediate High High Ultra Ultra-

  • High

High E Ebeam

beam [A

[A GeV] GeV] SIS SIS FAIR FAIR NICA NICA SPS SPS RHIC RHIC LHC LHC

‚ ‚Mixed Mixed‘ ‘ phase: phase: hadrons (baryons, mesons) + hadrons (baryons, mesons) + quarks and gluons quarks and gluons || || In In-

  • medium effects

medium effects Chiral symmetry restoration Chiral symmetry restoration Phase transition to sQGP Phase transition to sQGP Critical point in the QCD phase Critical point in the QCD phase diagram diagram QGP: quarks and gluons QGP: quarks and gluons || || Properties of sQGP Properties of sQGP

BM@N BM@N

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Wolfgang Cassing Wolfgang Cassing (Giessen Univ.) (Giessen Univ.) Volodya Konchakovski Volodya Konchakovski (Giessen Univ.) (Giessen Univ.) Olena Linnyk Olena Linnyk (Giessen Univ.) (Giessen Univ.) Elena Bratkovskaya Elena Bratkovskaya (FIAS & ITP Frankfurt Univ.) (FIAS & ITP Frankfurt Univ.) Vitalii Ozvenchuk Vitalii Ozvenchuk (HGS (HGS-

  • HIRe, FIAS & ITP Frankfurt Univ.)

HIRe, FIAS & ITP Frankfurt Univ.) Rudy Marty Rudy Marty (FIAS, Frankfurt Univ.) (FIAS, Frankfurt Univ.) Hamza Berrehrah Hamza Berrehrah (FIAS, Frankfurt Univ.) (FIAS, Frankfurt Univ.) Daniel Cabrera Daniel Cabrera (ITP&FIAS, Frankfurt Univ.) (ITP&FIAS, Frankfurt Univ.) External Collaborations: External Collaborations: SUBATECH, Nantes Univ. : SUBATECH, Nantes Univ. : J Jö örg Aichelin rg Aichelin Christoph Hartnack Christoph Hartnack Pol Pol-

  • Bernard Gossiaux

Bernard Gossiaux Texas A&M Univ.: Texas A&M Univ.: Che Che-

  • Ming Ko

Ming Ko JINR, Dubna: JINR, Dubna: Vadim Voronyuk Vadim Voronyuk Viatcheslav Toneev Viatcheslav Toneev Kiev Univ.: Kiev Univ.: Mark Gorenstein Mark Gorenstein Barcelona Univ. Barcelona Univ. Laura Tolos, Angel Ramos Laura Tolos, Angel Ramos Wayne State Uni. Wayne State Uni. Sergei Voloshin Sergei Voloshin

PHSD group PHSD group