Download - Heavy Ion Physics at NICA Simulations G.Musulmanbekov, V. Toneev and the Physics Group on NICA

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Page 1: Heavy Ion Physics at NICA Simulations G.Musulmanbekov, V. Toneev and the Physics Group on NICA

Heavy Ion Physics at NICASimulations

G.Musulmanbekov, V. Toneevand the Physics Group on NICA

Page 2: Heavy Ion Physics at NICA Simulations G.Musulmanbekov, V. Toneev and the Physics Group on NICA

Search for signals of Phase Transition in Au + Au collisions at √sNN = 3 – 9 GeV

Motivation

• The main goal of the NICA experiment is to study the behaviour of nuclear matter in vicinity of the QCD critical endpoint.

• To extract information on the equation-of-state of baryonic matter at high densities.

• Search for signals of Phase Transition in Au + Au collisions at √sNN = 3 – 9 GeV

Page 3: Heavy Ion Physics at NICA Simulations G.Musulmanbekov, V. Toneev and the Physics Group on NICA

Search for signals of Phase Transition in Au + Au collisions at √sNN = 3 – 9 GeV

Signatures of Possibile Phase Transition :

o Strange particle enhancement

o Hard spectrum of strange mesons

o Charmonium suppression

o Dielectron mass spectrum enhancement at the range 0.2 – 0.6 GeV/c

Page 4: Heavy Ion Physics at NICA Simulations G.Musulmanbekov, V. Toneev and the Physics Group on NICA

Search for signals of Phase Transition in Au + Au collisions at √sNN = 3 – 9 GeV

Observables :

• Global characteristics of identified hadrons, including strange baryons

• Strange to non-strange particles ratio

• Transverse momentum spectra

• Fluctuations in multiplicity and transverse momenta

• Directed and elliptic flows

• Particle correlations (femtoscopy, HBT correlations)

• Dilepton spectra

Page 5: Heavy Ion Physics at NICA Simulations G.Musulmanbekov, V. Toneev and the Physics Group on NICA

Search for signals of Phase Transition in Au + Au collisions at √sNN = 3 – 9 GeV

Simulation Tools :

• UrQMD 1.3, UrQMD 2.2o 104 central events at 3, 3.8, 5, 7, 9 GeVo 105 min bias events at 3, 3.8, 5, 7, 9 GeV

• FastMCo 104 central events at 3, 5, 7, 9 GeV

• PLUTO

o 106 central events at 3, 5, 7, 9 GeV

Page 6: Heavy Ion Physics at NICA Simulations G.Musulmanbekov, V. Toneev and the Physics Group on NICA

Mean multiplicities in Au-Au collisions Simulated by UrQMD min.bias events 

Page 7: Heavy Ion Physics at NICA Simulations G.Musulmanbekov, V. Toneev and the Physics Group on NICA

Mean multiplicities in Au-Au collisions Simulated by UrQMD central collisions (b ≤ 3 fm) 

Page 8: Heavy Ion Physics at NICA Simulations G.Musulmanbekov, V. Toneev and the Physics Group on NICA

Mean multiplicities in Au-Au collisions Simulated by UrQMD central collisions (b ≤ 3 fm) 

Page 9: Heavy Ion Physics at NICA Simulations G.Musulmanbekov, V. Toneev and the Physics Group on NICA

Mean multiplicities in Au-Au collisions Simulated by UrQMD central collisions (b ≤ 3 fm) 

Page 10: Heavy Ion Physics at NICA Simulations G.Musulmanbekov, V. Toneev and the Physics Group on NICA

Simulated charged multiplicity distributionsin central collisions (b < 3fm)

Page 11: Heavy Ion Physics at NICA Simulations G.Musulmanbekov, V. Toneev and the Physics Group on NICA

Simulated charged pseudorapidity distributions in central collisions (b < 3fm)

Page 12: Heavy Ion Physics at NICA Simulations G.Musulmanbekov, V. Toneev and the Physics Group on NICA

Simulated charged pseudorapidity distributions in central collisions (b < 3fm)

MPD-2 < η < 2

Page 13: Heavy Ion Physics at NICA Simulations G.Musulmanbekov, V. Toneev and the Physics Group on NICA

Simulated charged pseudorapidity distributions in central collisions (b < 3fm)

MPD-1 < η < 1

Page 14: Heavy Ion Physics at NICA Simulations G.Musulmanbekov, V. Toneev and the Physics Group on NICA

Strange Baryons Yield

Table: Marked hyperons are accessible through their decays into charged hadrons

Page 15: Heavy Ion Physics at NICA Simulations G.Musulmanbekov, V. Toneev and the Physics Group on NICA

Accessible Hyperons

Mass(GeV/c2) Lifetime cτ (cm) Multiplicity Decay channel

BR(%) Registration efficiency (%)|p| > 0.1 GeV/c

-1 < y < 1

ΛΞ-

Ω-

1.1161.3211.672

7.894.912.46

39.81.210.03

p + π-

Λ + π-

Λ + K-

63.999.967.8

1685

Page 16: Heavy Ion Physics at NICA Simulations G.Musulmanbekov, V. Toneev and the Physics Group on NICA

Accessible Hyperons

Λ → pπ- Ξ- → Λπ- → pπ- π- Ω- → ΛK- → pK- π-

Page 17: Heavy Ion Physics at NICA Simulations G.Musulmanbekov, V. Toneev and the Physics Group on NICA

Strange to non-Strange ratios in central collisions

“Horn” Effect

<π- >/<π+>Au+Au/Pb+Pb, central

<K+ >/<π+>Au+Au/Pb+Pb, central

Page 18: Heavy Ion Physics at NICA Simulations G.Musulmanbekov, V. Toneev and the Physics Group on NICA

Strange to non-Strange ratios in central collisions

“Horn” Effect

Page 19: Heavy Ion Physics at NICA Simulations G.Musulmanbekov, V. Toneev and the Physics Group on NICA

Strange to nonStrange ratios in central collisions

Page 20: Heavy Ion Physics at NICA Simulations G.Musulmanbekov, V. Toneev and the Physics Group on NICA

Strange to nonStrange ratios in central collisions

Page 21: Heavy Ion Physics at NICA Simulations G.Musulmanbekov, V. Toneev and the Physics Group on NICA

Strange to nonStrange ratios in central collisions

Page 22: Heavy Ion Physics at NICA Simulations G.Musulmanbekov, V. Toneev and the Physics Group on NICA

Transverse Mass Spectra of Mesonsin central collisions

T

m

dm

dN

mT

TT

exp1

T – inverse slope

Page 23: Heavy Ion Physics at NICA Simulations G.Musulmanbekov, V. Toneev and the Physics Group on NICA

Transverse Mass Spectra of Mesonsin central collisions

Page 24: Heavy Ion Physics at NICA Simulations G.Musulmanbekov, V. Toneev and the Physics Group on NICA

Transverse Mass Spectra of Mesonsin central collisions

Page 25: Heavy Ion Physics at NICA Simulations G.Musulmanbekov, V. Toneev and the Physics Group on NICA

Scaled multiplicity variances

i

ii

N

NN22

ω (h+)

ω (h-)

ω (hch)

Page 26: Heavy Ion Physics at NICA Simulations G.Musulmanbekov, V. Toneev and the Physics Group on NICA

Scaled multiplicity variancesNA49 results

NA49 result: Measured scaled variances are close to the Poisson one – close to 1!No sign of increased fluctuations as expected for a freezeout near the critical point of strongly interacting matter was observed.

Page 27: Heavy Ion Physics at NICA Simulations G.Musulmanbekov, V. Toneev and the Physics Group on NICA

Transverse momentum fluctuations

To exclude trivial fluctuations from consideration the following variable is used:

For the system of independently emitted particles (no inter-particle correlations) Фpt

goes to zero.

Page 28: Heavy Ion Physics at NICA Simulations G.Musulmanbekov, V. Toneev and the Physics Group on NICA

Directed flow v1 & elliptic flow v2

x

zNon-central Au+Au collisions:

Interactions between constituents leads to a pressure gradients => spartial asymmetry is converted in asymmetry in momentum space

=> collective flows

22

22

yx

yx2

T

x1

21TTTT

pp

ppv

p

pv

...)cos(22v)cos(2v12π

1

dpdyp

dN

ddpdyp

dN

- directed flow

- elliptic flowV2>0 indicates in-plane emission of

particlesV2<0 corresponds to out-of-plane

emission (squeeze-out perpendicular to the reaction plane)

Page 29: Heavy Ion Physics at NICA Simulations G.Musulmanbekov, V. Toneev and the Physics Group on NICA

Direct flow Au + Au collisions at √sNN = 7GeV, b = 5 – 9 fm

Page 30: Heavy Ion Physics at NICA Simulations G.Musulmanbekov, V. Toneev and the Physics Group on NICA

Direct flow slopeCollision Energy Dependence

Au + Au, b = 5 – 9 fm

Page 31: Heavy Ion Physics at NICA Simulations G.Musulmanbekov, V. Toneev and the Physics Group on NICA

Elliptic flow Au + Au collisions at √sNN = 7GeV, b = 5 fm

Page 32: Heavy Ion Physics at NICA Simulations G.Musulmanbekov, V. Toneev and the Physics Group on NICA

Elliptic flow Collision Energy Dependence

Au+Au/Pb+Pb, b = 5 – 9 fm

Page 33: Heavy Ion Physics at NICA Simulations G.Musulmanbekov, V. Toneev and the Physics Group on NICA

Sergey Panitkin

qout

qside

qlong

HBT interferometry

Rsi

de

R long

Rout

x1

x2

12 ppq

p1

p2

q

12 pp2

1k

Two-particle interferometry: p-space separation space-time separation

HBT: Quantum interference between identical particles

pairsevent mixed

pairsevent real

)(P)(P

),(P),(

21

2121

pp

ppppC

2long

2long

2side

2side

2out

2out)(1),(

RqRqRqekkqC

q (GeV/c)q (GeV/c)

C (

q)C

(q)

11

22R

1~

– Final-state effects (Coulomb, strong) also can cause correlations, need to be accounted for

Gaussian model (3-d):

Page 34: Heavy Ion Physics at NICA Simulations G.Musulmanbekov, V. Toneev and the Physics Group on NICA

HBT interferometry

)qRqRqRexp(1)q,q,q(C 2S

2S

2O

2O

2L

2LLS0

Page 35: Heavy Ion Physics at NICA Simulations G.Musulmanbekov, V. Toneev and the Physics Group on NICA

HBT interferometry

Page 36: Heavy Ion Physics at NICA Simulations G.Musulmanbekov, V. Toneev and the Physics Group on NICA

HBT interferometry

Page 37: Heavy Ion Physics at NICA Simulations G.Musulmanbekov, V. Toneev and the Physics Group on NICA

Dilepton Spectra

Page 38: Heavy Ion Physics at NICA Simulations G.Musulmanbekov, V. Toneev and the Physics Group on NICA

Dilepton Spectra

Page 39: Heavy Ion Physics at NICA Simulations G.Musulmanbekov, V. Toneev and the Physics Group on NICA

Dilepton Spectra

Page 40: Heavy Ion Physics at NICA Simulations G.Musulmanbekov, V. Toneev and the Physics Group on NICA

Dilepton Spectra

Page 41: Heavy Ion Physics at NICA Simulations G.Musulmanbekov, V. Toneev and the Physics Group on NICA

Dilepton Spectra

Page 42: Heavy Ion Physics at NICA Simulations G.Musulmanbekov, V. Toneev and the Physics Group on NICA

Conclusions

New simulation codes which take into accountphase transitions of deconfinement and/or chiral symmetry restoration are needed.

Page 43: Heavy Ion Physics at NICA Simulations G.Musulmanbekov, V. Toneev and the Physics Group on NICA

Thank you!