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1 28 July – 6 August 2014, Kolymbari, Crete, Greece
STAR Highlight on Heavy Ion Physics
Shusu Shi for the STAR collaboration
Lawrence Berkeley National Laboratory
The 3rd International Conference on New Frontiers in Physics 2014
2 28 July – 6 August 2014, Kolymbari, Crete, Greece
Ø Introduction
Ø STAR Detectors
Ø Recent Results Ø Top energy collisions at RHIC - Study the medium properties Ø Beam Energy Scan at RHIC - QCD phase boundary and critical point
Ø Summary/Outlook
Outline
3 28 July – 6 August 2014, Kolymbari, Crete, Greece
Large acceptance at mid-rapidity! Time Projection Chamber: Full azimuthal coverage, (|η|<1.0)
Excellent particle identification!
STAR Detectors
4 28 July – 6 August 2014, Kolymbari, Crete, Greece
2 2
2 2
y xy x
ε< − >
=< + >
v2 =< cos2ϕ >, ϕ = tan−1(pypx)
Elliptic flow => Ø Initial spatial anisotropy (eccentricity ε) -> final momentum anisotropy v2 by interactions among constituents
Ø Self-quenching with time Ø Sensitive to the early stages of the system evolution
Good probe of the early stage of the collision.
partonic hadronic
Elliptic Flow (v2)
5 28 July – 6 August 2014, Kolymbari, Crete, Greece
Ø RHIC delivered the U+U collisions in order to study geometry effects Ø Tip-tip and body-body enhanced samples selected via ZDC-mult cut Ø IP-Glasma model matches the data better Bjoern Schenke, et al. arXiv:1403.2232 Maciej Rybczyński, et. al. PRC87,044908(2013)
v2 in U+U Collisions
more overlapping fewer spectators
Dashed boxes are systematic errors
ZDC (%)
Slo
pe
6 28 July – 6 August 2014, Kolymbari, Crete, Greece
Ø Event-by-Event fluctuations ε3 -> v3 Ø The number of constituent
quark scaling does not work for v3
Ø Hydro inspired (nq)i/2, i=3, seems to work for 200 GeV collisions up to (mT-m)/nq ~ 1 GeV/c2
P. Huovinen, Phys. Lett. B503, 58 (2001) R. Lacey, J. Phys. G38, 124048(2011)
Triangular Flow v3
7 28 July – 6 August 2014, Kolymbari, Crete, Greece
0 2 4 6 8
-2dy
) (G
eV/c
)T
dp Tp/2ev
N/(N
2 d -710
-410
-110
210 )/2, |y| < 10D+0U+U 193 GeV (D0-80%
20]×0-10% [5]×10-40% [
40-80% [/2]
2]×+D* [0p+p D
Au+Au 200 GeV
for Au+Au 200GeV�binN�p+p Levy scaled by
for U+U 193GeV�binN�p+p Levy scaled by
STAR Preliminary
(a)
Transverse
0.51
1.52 40-80% (b)
STAR Preliminary
AA R0 D 0.5
11.5
2 10-40% (c)
0 2 4 6 8
0.51
1.52
0-10% (d)
(GeV/c)T
Momemtum ppT (GeV/c)
Au+Au@200 GeV: submitted to PRL, arXiv:1404.6185
D0 R
AA
Open Heavy Flavor
Particle production in A+A
Particle production in p+p
Average number of binary collisions in A+A
Ø Large suppression at high pT indicates strong charm-medium interactions Ø Enhancement at pT ~ 0.7-2 GeV/c: described by models with charm quark coalescence with light quarks
David Tlusty: August 6 [parallel 2]
8 28 July – 6 August 2014, Kolymbari, Crete, Greece
partN0 100 200 300 400
AA
R
00.20.40.60.8
11.21.41.61.8
2200 GeV theoretical curve62.4 GeV theoretical curve39 GeV theoretical curve
uncertaintycollNp+p uncertainty 62.4 GeVp+p uncertainty 39 GeVp+p 200 GeV(statistics)
Au+Au 200 GeV
Au+Au 62.4 GeV
Au+Au 39 GeV
U+U 193 GeV
Ø Suppression increases with collision centrality Ø Similar suppression in U+U and Au+Au collisions Ø Weak beam energy dependence of J/ψ RAA X.B. Zhao et al., PRC82, 064905(2010) L. Yan et al., PRL97, 232301(2006)
J/ψ STAR Preliminary
Quarkonia
Barbara Trzeciak: August 2 [parallel 4]
9 28 July – 6 August 2014, Kolymbari, Crete, Greece
BES-I
Beam Energy Scan at RHIC
Data: 5% Au+Au collisionsA. Adronic, et al.J. Cleymans, et al.
10 100 10000
50
100
150
200
Tem
pera
ture
Tch
(MeV
)
Baryonic Chemical Potential µB (MeV)
Au+Au Collisions at RHIC //STAR//11 BESII//R
eferences//03/plot2_cfo_March2014.kum
ac//
LGT: S. Gupta, et al.LGT: Z. Fodor, et al.
(TC = 170 MeV)
Observables:
Phase boundary Charge separation; v2 - NCQ scaling 1st order phase transition Directed flow v1 Critical point Fluctuations Chiral symmetry restoration Di-lepton production
Statistical-Thermal Model
STAR Preliminary
√sNN (GeV) 7.7 11.5 14.5 19.6 27 39
µB (MeV) 420 315 260 205 155 115
Study QCD Phase Structure! Year 2014
Daniel McDonald: July 29 [FAIR workshop]
10 28 July – 6 August 2014, Kolymbari, Crete, Greece
Ø The difference between particles and anti-particles increases with decreasing beam energy – NCQ scaling breaks
Ø Model comparison Ø Hydro + Transport (UrQMD): consistent with baryon data Ø Nambu-Jona-Lasino (NJL) model (partonic + hadronic potential): hadron splitting consistent
J. Steinheimer, V. Koch, and M. Bleicher PRC86, 44902(2013); J. Xu, et al., PRL112, 012301(2014)
0
0.01
0.02
0.03
0.04
0 100 200 300 400
pR
K/
Exp. data Hybrid model
p
K
/
0-80% Au + Au Collisions at RHIC
Baryonic Chemical Potential µB (MeV)
200 39 27 19.6 11.5 7.7 (GeV)
v 2(pa
rt.) -
v2(
anti-
part.
)
0 100 200 300 400
RV=0.5
RV=1.1
pR
K/
Exp. data NJL model
200 39 27 19.6 11.5 7.7 (GeV)
(b)(a)
(GeV)NNs0 20 40 60
)X( 2
(X)-v
2v
0
0.02
0.04
0.06
0.08Au+Au, 0-80%-sub EPη
+Ξ--Ξ
pp-Λ-Λ --K+K
-π-+π
Particle vs. Anti-particle v2
STAR: Phys. Rev. Lett. 110 (2013) 142301
11 28 July – 6 August 2014, Kolymbari, Crete, Greece
Ø Hydro calculation with 1st order phase transition motivates the study
Ø Net-proton slope changes sign twice EOS softest point? Ø UrQMD fails to reproduce the data
Ø BESII improvement: Improved reaction plane determination
Systematic centrality-dependent analysis STAR: PRL112, 162301(2014) H. Stoecker, NPA750, 121(2005)
Directed Flow v1: Softest Point
dv1/dy: the slope of directed flow versus rapidity near mid-rapidity
12 28 July – 6 August 2014, Kolymbari, Crete, Greece
SS -
OS
Ø H: CME contributions A. Bzdak et al., Lect. Notes Phys. 871, 501 (2013)
è Disappears at low energy hadronic interactions become dominant at √sNN ≤ 11.5 GeV D. Kharzeev. PLB633, 260 (2006) D. Kharzeev, et al. NPA803, 227(2008) (GeV)NNs
10 210 310
4 1
0×
) O
S -
HSS
(H
-1
0
1
2 30 - 60%
= 1g = 1.5g = 2g
BES II error projection
Au+Au Pb+Pb
STAR: PRL 113, 052302 (2014)
Charge Separation wrt Event Plane Chiral Magnet Effect + Local Parity Violation
STAR: PRL. 103, 251601(2009)
13 28 July – 6 August 2014, Kolymbari, Crete, Greece
0.4
0.6
0.8
1
[
[
[
[ [
[
[
[
[
[
[
[ [
[
Net
-pro
ton gm
2
(a) STAR net-proton data70 - 80% 0 - 5%
(|y|<0.5; 0.4<pT<0.8(GeV/c))
UrQMD (0 - 5%)Poisson
BESII error
-10
0
10
[
[
[
[
[
[
[
[
[
[
[
[ [ [
Net
-cha
rge gm
2
10 20 505 100 200
Colliding Energy 3sNN (GeV)
(b) STAR net-charge data70 - 80% 0 - 5%
(|d|<0.5; 0.2<pT<2.0(GeV/c))
NBD (0 - 5%)Poisson
Au + Au Collisions at RHIC
Non-monotonic behavior would be indicative of existence of CP Net-proton results:
Ø Deviations below Poisson for κσ2 at all energies. Relatively larger deviation at √sNN~20GeV
STAR: PRL112, 32302(2014)
Net-charge results:
Ø No non-monotonic behavior Ø More affected by resonance
decays
STAR: arXiv: 1402.1558
Higher statistics needed for collisions at √sNN < 20 GeV
Sensitive to critical point (ξ correlation length):
δN( )2 ≈ ξ 2, δN( )3 ≈ ξ 4.5, δN( )4 ≈ ξ 7
Sσ ≈χB3
χB2 ,κσ
2 ≈χB4
χB2
Higher Moments
14 28 July – 6 August 2014, Kolymbari, Crete, Greece
Ø Mee < 1.1 GeV/c2: Model results with in- medium broadened ρ are consistent with data.
Ø 1.1 < Mee < 3.0 GeV/c2: QGP thermal radiation Ø BES-II: high statistics R. Rapp: PoS CPOD13, 008(2013)
200GeV
19.6GeV
Di-electrons
BES: STAR Preliminary 200 GeV: PRL 113, (022301) 2014
Clean and penetrating probe! Do not suffer from strong interactions
15 28 July – 6 August 2014, Kolymbari, Crete, Greece
Ø Top Energy Heavy Ion Collisions - Initial Condition: U+U collisions: IP-Glasma results match data better - Hot and dense sQGP: Heavy flavor hadron RAA: large suppression for D mesons at high pT
Ø RHIC Beam Energy Scan Program √sNN ≥ 39 GeV: partonic interactions dominant √sNN ≤ 11.5 GeV: hadronic interactions dominant
Ø Outlook - Heavy flavor program with new upgrade Heavy Flavor Tracker and Muon Telescope Detector - RHIC BES-II: Focus on √sNN ≤ 20 GeV region
Summary/Outlook
2013 2014 2015 2016 2017 2018 2019
Charm; Di-lepton; sQGP properties
BESII HFT/MTD e-Cooling, iTPC
16 28 July – 6 August 2014, Kolymbari, Crete, Greece
Heavy Flavor Tracker (HFT) Physics goal: Precision measurement of heavy quark hadron production in heavy ion collisions
Collected 1.2 B Au+Au at 200 GeV events in year 2014
HFT and MTD
Muon Telescope Detector (MTD): Physics goal: Heavy Quarkonia – Upsilon states Took 12 nb-1 Au+Au collisions at 200 GeV in year 2014 for quarkonium physics
Both Fully installed in Run14!
Spyridon Margetus: August 5 [parallel 5]
17 28 July – 6 August 2014, Kolymbari, Crete, Greece
BES II Electron cooling + longer beam bunches for BES II factor 4-15 improvement in luminosity compared with BES I Detector upgrade Ø Event Plane Detector important for flow and fluctuation analyses Ø iTPC upgrade increases TPC acceptance to ~1.7 in η; improves dE/dx resolution Fixed target program extends STAR’s physics reach to region of compressed baryonic matter
With electron cooling and long beam bunches
With electron cooling
BES I performance
Grazyna Odyniec: August 4 [Plenary 5]