event anisotropy in high-energy heavy-ion collisions at rhic
DESCRIPTION
Event anisotropy in high-energy heavy-ion collisions at RHIC ShinIchi Esumi Inst. of Physics, Univ. of Tsukuba elliptic flow and nuclear suppression factor identified hadron v 2 - PowerPoint PPT PresentationTRANSCRIPT
JPS/DNP 2005 Sep. Maui ShinIchi Esumi, Univ. of Tsukuba 1
Event anisotropy in high-energy heavy-ion collisions at RHIC
ShinIchi Esumi Inst. of Physics, Univ. of Tsukuba
elliptic flow and nuclear suppression factor identified hadron v2
v2/RAA(quark coalescence or hydro) electron v2/RAA(charm quark) inclusive , 0 v2 (direct v2/RAA) (eccentricity) scaling jet correlation and v2
JPS/DNP 2005 Sep. Maui ShinIchi Esumi, Univ. of Tsukuba 2
x
zNon-central Collisions
initial collision geometry
pressure/density gradient, radial/elliptic expansion
final momentum anisotropy
Σ wi*sin(ni) tan(nn) = Σ wi*cos(ni)
y
x
reaction plane angle : n
i-n|
2nd harmonic amplitude : v2
v2
JPS/DNP 2005 Sep. Maui ShinIchi Esumi, Univ. of Tsukuba 3
2x1=23x2=63x3=93x3=91x2=21x2=2
total 30 collisions12 + 11
total 23 participant nucleons
spectators
Npart : number of participant participant scaling
Ncoll : number of binary collision binary scaling
impactparameter : b
y
x
b
x
z
R AA = yield (A+A)
<Ncoll> yield (p+p)
R CP =yieldCentral / <Ncoll>Central
yieldPeripheral / <Ncoll>Periheral
RAA , RCP
relative yield in A+A collisions normalized by p+p yield times number ofbinary collisions
JPS/DNP 2005 Sep. Maui ShinIchi Esumi, Univ. of Tsukuba 4
SMD/ZDC
BBC
Reaction plane detectors
participant elliptic R.P.
spectator directed R.P.
MVD
JPS/DNP 2005 Sep. Maui ShinIchi Esumi, Univ. of Tsukuba 5
SMD1vsSMD2BBC1vsBBC2 SMDvs BBC
BBC1vs
BBC2
back-to-back back-to-back spectator neutrons vss from participants are flowing opposite.
MVD1vs
MVD2 BBCvs
MVD
directed plane
elliptic plane
beam linereaction plane
neutron spectator
charged particles(pions) at mid
beam
JPS/DNP 2005 Sep. Maui ShinIchi Esumi, Univ. of Tsukuba 6
Identified hadron v2
hydro dynamic behavior at low pTbaryon/meson difference at high pT
QM05 PHENIX QM05 STAR
JPS/DNP 2005 Sep. Maui ShinIchi Esumi, Univ. of Tsukuba 7
-meson v2
mass scaling or number of quark scaling?baryon/meson (number of quark) differencehydro dynamic behavior : m-meson ~ mproton
early hadronic freeze-out for multi-strangeness hadrons
QM05 PHENIX QM05 STAR
Ξ+ΞΩ+Ω
__
need more data/beam
JPS/DNP 2005 Sep. Maui ShinIchi Esumi, Univ. of Tsukuba 8
Nuclear modification factor : RCP
clear separation between baryon group / meson group including as well as ,K,p
JPS/DNP 2005 Sep. Maui ShinIchi Esumi, Univ. of Tsukuba 9
Number of quark scaling of v2
rather good description above 1GeV/c in quark pT
remaining mass dependence at lower pT regionv2 is already formed during quark phase before hadronizationadditional hadronic flow might be there after hadronization
QM05 PHENIX QM05 STAR
JPS/DNP 2005 Sep. Maui ShinIchi Esumi, Univ. of Tsukuba 10
(3) q_hat = 14 GeV2/fm
(2) q_hat = 4 GeV2/fm
(1) q_hat = 0 GeV2/fm
(4) dNg / dy = 1000
Non-photonic electron (charm origin) RAA compared with 0 RAA
Non-photonic electron is less suppressed compared with 0, but it is still a significant suppression RAA~ 0.3 at higher pT region 4~5GeV/c
non-photonic electron v2 is similar with other hadronsnon-photonic electron v2 is similar with other hadronsat low pat low pTT but smaller at higher p but smaller at higher pTT region 4~5GeV/c region 4~5GeV/c
photonic electron v2 originated from photonic electron v2 originated from 00
is above is above 00 v2 at low pT and similar to v2 at low pT and similar to 00 v2 at high pT and v2 at high pT and subtracted already.subtracted already.
JPS/DNP 2005 Sep. Maui ShinIchi Esumi, Univ. of Tsukuba 11
B. Zhang et al.nucl-th/0502056
non-photonic electron : charm (+beauty) RAA and v2
very significant suppression at higher pT some difference between experiments at higher pT almost same as 0 suppression above 5GeV/c which needs to be solved. D-meson flows (+ve v2), should determine charm v2
b contributionless suppressionless interaction
b contributionless flowless thermalized
I’m very much looking forward to hearing following electron v2 talks!!
JPS/DNP 2005 Sep. Maui ShinIchi Esumi, Univ. of Tsukuba 12
Direct photons are not suppressed
RAA is about 1.0 high pT, 0 ratio > 1 at high pTDirect photon contribution is significant at high pT and atcentral collisions compared to the inclusive photon yieldfrom the known hadronic sources.
JPS/DNP 2005 Sep. Maui ShinIchi Esumi, Univ. of Tsukuba 13
inclusive and 0 v2
nucl-ex/0508019
v2 of direct photon gives complimentary information in understanding the origin of binary scaled direct photon production.
Bresmsrahlung, because of largerenergy loss v2 < 0
fragmentation
in vacuum, from escapedpartonv2 > 0
JPS/DNP 2005 Sep. Maui ShinIchi Esumi, Univ. of Tsukuba 14
try to extract direct v2
v2direct =
R v2inclusive – v2
b.g.
R – 1
v2b.g. : expected v2 from hadronic decays
if v2direct = 0 R =
v2inclusive
v2b.g
nucl-ex/0508019
JPS/DNP 2005 Sep. Maui ShinIchi Esumi, Univ. of Tsukuba 15
QM05 : Phenix preliminary run4inclusive and 0 v2
0
inclusive
v2
0 5 pT (GeV/c) 10
0-10 % 10-20 %
30-40 %
50-60 %40-50 %
20-30 %
JPS/DNP 2005 Sep. Maui ShinIchi Esumi, Univ. of Tsukuba 16
Low pT direct can be extracted in a different way for both pT distribution and v2.
better accuracy at low pT might be expected.
JPS/DNP 2005 Sep. Maui ShinIchi Esumi, Univ. of Tsukuba 17
dNch/d scales with Npart for both Au+Au / Cu+Cu
JPS/DNP 2005 Sep. Maui ShinIchi Esumi, Univ. of Tsukuba 18
RAA scales with Npart for both Au+Au / Cu+Cu
JPS/DNP 2005 Sep. Maui ShinIchi Esumi, Univ. of Tsukuba 19
<v2> (||<2)
black : Au+Au
red : Cu+Cu
RQMDv2.4
v2 does NOT scale with Npart
for obvious reason
----- Geometry -----
true R.P.
participant R.P.
with true R.P.
if use all participants to define its axis and its deformation, maximum auto-correlation in definition?
JPS/DNP 2005 Sep. Maui ShinIchi Esumi, Univ. of Tsukuba 20
Participant eccentricity includes initial statistical fluctuation of and its axis, while experimental v2 and reaction plane (from participants with the 2nd moment axis) includes all fluctuations until final particle productions.
JPS/DNP 2005 Sep. Maui ShinIchi Esumi, Univ. of Tsukuba 21
Lesson from PHOBOS should also be considered when comparing between experiments especially for light system.
Npart. scalingNcoll. scalingecc. scaling
Au+AuCu+CuSi(Cu)+Au
v2 RAA jet/HBT(R.P.)
The difference between 2nd and 4th order cumulant results differ especially for Cu+Cu.
QM05 PHENIX QM05 STAR
238U + 238USi + Au
JPS/DNP 2005 Sep. Maui ShinIchi Esumi, Univ. of Tsukuba 22
Au +Au 200 GeV
STAR
prelimi
nary
ZDC/SMD spectator v1
spectator directed R.P.
participant elliptic R.P.
1st moment R.P. (SMD/ZDC, BBC, FTPC)
of participant with axis from spectator : yet another needed? Cu+Cu w.r.t. SMD/ZDC (spectator directed) R.P. needed, it can be different with participant elliptic R.P.
QM05 PHOBOS
QM05 STAR
JPS/DNP 2005 Sep. Maui ShinIchi Esumi, Univ. of Tsukuba 23
ISMD 2005
UrQMD
We should not forget that hadronic cascade can generate apparent number of quark scaling without quark coalescence, although the magnitude of v2 is about a half of experimental data.
origin of this apparent scaling needs to be understood
JPS/DNP 2005 Sep. Maui ShinIchi Esumi, Univ. of Tsukuba 24
High pT away-side jet suppression
softening of associated pT distribution
modification of jet shape at mid-pT
QM05 : Phenix preliminary
JPS/DNP 2005 Sep. Maui ShinIchi Esumi, Univ. of Tsukuba 25
STAR Preliminary
Au+Au, 0-5%
pT(assoc) > 2 GeV/c
re-appearance (escaped) of high pT back-to-back jet
pT
pT
JPS/DNP 2005 Sep. Maui ShinIchi Esumi, Univ. of Tsukuba 26
STAR Preliminary 8 < pT(trig) < 15 GeV/c
pT(assoc)>6 GeV
re-appearance (escaped) of high pT back-to-back jet
centrality
system/centrality
PHENIX Preliminary
JPS/DNP 2005 Sep. Maui ShinIchi Esumi, Univ. of Tsukuba 27
0 (rad)
pTtrigger(h) > 3GeV/c
1< pTassociated(h) <2GeV/c
PHENIX preliminary
jet shape w.r.t. R.P.source of v2 at high pT
v4 effects need to be consideredjet v2 = b.g.(thermal) v2 extract jet shape or jet v2
in-plane pairin between pairout-of-plane pair
jet y
ield
(a.
u.)
PHENIX preliminary
JPS/DNP 2005 Sep. Maui ShinIchi Esumi, Univ. of Tsukuba 28
Summary
identified particles, , e, v2
partonic flow ? heavy quark v2 ? direct photon production ?
Npart. , Ncoll. , ecc.scaling
test with asymmetric collisions ?
jet correlation and v2
jet shape w.r.t. R.P. or jet v2 ?
RAAv2
proton pion electron photon
pT pT
1
0
0
0.1
0
0
jet shape
JPS/DNP 2005 Sep. Maui ShinIchi Esumi, Univ. of Tsukuba 29
JPS/DNP 2005 Sep. Maui ShinIchi Esumi, Univ. of Tsukuba 30
0 1 2 3 4 5
v 2
0.00
0.05
0.10
0.15
0.20
0.25
0.30 s 200 GeVNNAu Au
0SKp
fsTy
5 < Centrality < 30 %
K
(STAR)
(PHENIX)
(STAR)
(PHENIX)
(PHENIX)