SPS????????????? Mean-Field effects at SPS energies @ ???? RCNP, 4 Nov. 2004 PowerPoint PPT Presentation

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Title: SPS????????????? Mean-Field effects at SPS energies @ ???? RCNP, 4 Nov. 2004


1
SPS?????????????Mean-Field effects at SPS
energies _at_ ???? RCNP, 4 Nov. 2004
  • ??? ?? ?? (M. Isse)
  • ?????
  • ?? ?? ?? (N. Otuka)
  • IOP P.K.?? (P.K. Sahu)
  • Frankfurt U. ?? ? (Y. Nara)
  • ??? ?? ? (A. Ohnishi)

2
???????
  • ????
  • ??????(?????)
  • ???????????????????
  • ?????
  • ????????JAM
  • ????????????
  • ??
  • ?AGS E895, E877????ltpxgt,v2
  • ?SPS NA49????v1,v2
  • ?????????????
  • ???

3
Introduction
  • Heavy-ion collisions provides information about
    nuclear equation of state (EOS).
  • EOS gives the some static thermal property of
    nuclei (B.E., radius, )
  • We have to rely mostly on theoretical estimates
    to know the high density and/or high temperature
    EOS.
  • Other transport models shows the collective flows
    are very sensitive to the EOS.
  • Strong collective flows are measured in 1984 at
    Bevalac. Followed Experiments also show radial or
    sideward expansions.
  • Momentum dependence on collective flows are
    studied from around 1990. In order to distinguish
    momentum and density dependence, we have to
    investigate wide incident energy range.

4
Collective Flow Measurements in Heavy-Ion
Collisions
Accelerator Inc. Energy (AGeV) Particle Year
GSI-SIS(FOPI) LBNL-Bevalac(EOS) 0.12 Ni,Nb, Au,Pb 1986
BNL-AGS (E877) 11 Au 1993
CERN-SPS(NA49) 158,40, 20,30,60,80 Pb 1995
BNL-AGS (E895) 28 Au 1997
BNL-RHIC 6565,100100, 3131 Au 2000
5
Collective Flows
  • Anisotropic collective flows (ltpxgt, v1,v2)
    emerges in non-central collisions.
  • Very sensitive to the EOS.

6
Previous Works (1)
P.K.Sahu, W.Cassing, U.Mosel and A.Ohnishi, NPA
672(2000),376
  • F is the slope of ltpxgt and normalized y at
    mid-rapidity.
  • F decreases above 2 AGeV as a function of
    incident energy.
  • Small F means small pressure to sideward
    direction, namely the created matter is soft.
  • Boltzmann equation based model (RBUU) well
    reproduce the data below 11 AGeV (SIS to AGS
    energies).

7
Previous Works (2)
  • Momentum dependent mean field is necessary to
    describe heavy ion collisions from SIS to AGS
    energies (0.111 A GeV)
  • This work also used Boltzmann Equation based MF
    model
  • P.Danielewicz, R.Racey, W.G.Lynch, Science
    298(2002),1592

8
Previous Works (3)
  • Momentum dependent soft mean field well describe
    azimuthal anisotropy in 0.4 A GeV AuAu
    collisions.
  • Azimuthal dependence of mean kinetic energy
    can be fit via ltEkingtE0kin DEkincos2f .
  • FOPI Collaboration and P. Danielewicz, PRL
    92(2004),072303

9
Motivation
  • Many previous succeeded works used Boltzmann
    equation based model to describe mean field(MF).
    We would like to take other approach.
  • Cascade model QMD type MF
  • MF effects in heavy-ion collisions are well
    studied up to AGS energies (Einclt11 A GeV).
  • Now anisotropic flow data in SPS energies are
    available.
  • NA49 Collab.(C. Alt et al), PRC
    68(2003),034903

10
Hadron-String Cascade JAM
  • JAM describes heavy-ion collision by multiplying
    hadron-hadron collision in the energy range of
    Einc 1-160 AGeV and over.
  • All established hadronic states with masses up to
    around 2 GeV with isospin and antiparticles.
  • Inelastic hadron-hadron collisions produce
    resonance at lower energies.
  • At higher energies(?s gt 24 GeV), color strings
    are formed and they decay into hadrons according
    to Lund string model PYTHIA.
  • At high energies(?s gt 10 GeV), multiple mini-jet
    production is included using eikonal formalism
    for pQCD.

Ref.Y.Nara et al.PRC61(2000),024901
11
Including Mean Field(MF)
  • To improve description of hadron-hadron binary
    collisions. MF works in evolution stage after
    collisions.
  • We adopt a framework of constraint Hmiltonian
    dynamics RQMD/S T.Maruyama et al. PTP
    96(1996),263 into JAM.
  • N-body Hamiltonian with MF and their time
    derivatives are analytically given.

12
Including Mean Field
  • We include density dependent potential with
    (without) momentum dependent potential MH,MS
    (H,S). They are parameterized to give
    saturation at ??0 and two type EOS. The
    curvature represents incompressibility.

13
Density dependent potential
  • First term is given as Skyrme type zero-range
    approximated interaction where ? f(r,p) dp
    ? (r).
  • a,b,g and Cex(k)are parameter to give saturation
    property.
  • Second term is a momentum dependent part.

14
Momentum dependent potential
  • Lorentzian type momentum dependent mean-field
    which simulates the exchange term of Yukawa
    potential.
  • The Schrödinger Equivalent Potential is a
    functional derivative of potential energy
    UdV/df.
  • This parameterization is chosen to reproduce real
    part of optical potential taken by Hama et al. of
    nucleon-nucleus collision experiments.

15
Including Mean Field
  • In the actual simulation we use these equations
    for each i-th particles.

16
Mean Field at AGS energies
  • Einc2-11 AGeV

17
Sideward Flowltpxgtvs y (Proton)
Comparison with AGS E895 data PRL 84(2000),5488
  • Mean momentum of sideward emitted particles in
    mid-central collisions.
  • Momentum dependent mean-field (MH,MS) well
    reproduces 2 to 8 AGeV data.
  • E895

18
Sideward Flowltpxgtvs y (Proton,Pion)
Comparison with AGS E877 data PRC 56(1997)3254
  • Mean momentum of sideward emitted particles in
    mid-central collisions.
  • Momentum dependent mean-field (MH,MS) well
    reproduces 2 to 8 AGeV data.
  • E877

19
Mean Field at SPS energiesComparison with SPS
NA49 data NA49 Collab.(C. Alt et al), PRC
68(2003),034903
  • Einc40 and 158 AGeV
  • Time step dt0.1
  • Nucleons feel MF
  • (resonance and other baryons, anti-baryons dose
    not feel MF)

20
Directed Flow v1 vs y (Proton)
Momentum dependent MF MH,MS also well reproduces
40 AGeV data. In 158 AGeV MH, MS show negative
slope at mid-rapidity, while density dependent MF
H,S show positive. The observed wiggle can be
explained in momentum dependent MF?
ltpxgt will be calculated via integrating v1 with
pT multiplicity weight as
21
Directed Flow v1 vs y (Pion)
We find that pions are emitted to escape nucleons
at mid-rapidity.
22
Directed Flow v1 vs PT (Proton)
  • We take ylt1.5 and averaged with the sign. NA49
    take 0ltylt2.1.
  • The reason of narrow range is to omit counting
    nucleons in spectator.
  • yproj2.234 (40AGeV)
  • yproj2.912(158AGeV)

23
Directed Flow v1 vs PT (Pion)
In 40 A GeV MS is good, although in 158 A GeV no
MF(CS) seems good.
24
Elliptic Flow v2 vs y (Proton)
All MF well suppress the proton v2.
25
Elliptic Flow v2 vs y (Pion)
All MF on nucleons also well suppress the pion v2.
26
Elliptic Flow v2 vs PT (Proton)
We take also ylt1.5 and averaged with the sign
as did in v1analysis. NA49 take 0ltylt2.1. We find
MH and MS well suppress v2.
27
Elliptic Flow v2 vs PT (Pion)
We find all MF give a bit over estimate at lower
pt region, but tendency is good.
28
Incident energy dependence of v2
  • Momentum dependent mean-field well describe the
    integrated negative proton elliptic flow at lower
    incident energies.

Proton
29
Discussion
  • Time scale to form flows
  • Conditions of MF
  • ?Which particle feels MF ?
  • (only Nucleons / all Baryons)
  • ? Timestep of the calculation
  • MF on higher(RHIC) energies

30
Time evolution
  • Einc40 AGeV, PbPb
  • 4ltblt8 fm collisions
  • ylt0.8yproj ,hadrons

V2 are formed gradually in a large time scale,
v1 is formed in a very short time. V2 can grow
without MF, v1 cannot.
31
MF for only Nucleons(N) or All Baryons(B) (1)
  • We compare different conditions in MS type MF on
    sideward flow.
  • Small difference between two time steps (N,0.1
    and N,0.5)
  • Large difference between MF included species
    (N,0.5 and B,0.5)

Pion
Proton
32
MF for only Nucleons(N) or All Baryons(B) (2)
  • We compare different conditions in MS type MF on
    sideward flow.
  • Visible difference between species (N,0.5 and
    B,0.5) (N,0.1 and N,0.5)

33
v2 of ?s62 AGeV (Preliminary)
(Einc2050 AGeV)
Proton
Pion
We expect MF effects even lower RHIC energies.
34
v2 vs pT
Proton
Pion
?s62
  • For experimentalists.
  • ?We want precise anisotropic flow study at lower
    RHIC energies as SPS-NA49 paper.

35
Summary
  • We investigate heavy-ion collisions from AGS to
    SPS energies (2158 AGeV) by using hadron-string
    cascade JAM with covariant mean-field model
    RQMD/S.
  • We adopt two-type of mean-field potentials which
    are momentum dependent and independent. The
    momentum dependent interaction improves the
    description well at SPS energies(40 and 158
    AGeV).
  • Mean Field between nucleons affects also pion
    distributions. It improve description.
  • Our results suggests momentum dependent
    interaction have essential role to form
    corrective flows. The nuclear incompressibility
    dose not vary resulting corrective flows so much.
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