Outline - Weizmann Institute of Science · c=0.34 ± 0.16 GeV/fm3 : central lowest energy 7.7 GeV...
Transcript of Outline - Weizmann Institute of Science · c=0.34 ± 0.16 GeV/fm3 : central lowest energy 7.7 GeV...
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Heavy ion collisions at lower energies: challenges and opportunities
Beam Energy Scan (BES I and II) from RHIC Lijuan Ruan
(Brookhaven National Laboratory)
Outline: • Introduction and Motivation
• Results from BES I
• Future perspectives with BES II
• Summary
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Map out the phase diagram
• disappearance of QGP signatures (QGP turn off) • first order phase transition • critical point • chiral symmetry restoration (not covered)
Particle spectra
• Global quantities: Tch, Tkin, µB, energy density, freeze-out volume… arXiv: 1701.07065
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Freeze-out parameters
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• At √sNN > 7 GeV, Tch > Tkin • At √sNN < 7 GeV, Tch ~ Tkin • Collective velocity increases as a function of √sNN.
Energy density
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• Bjorken Energy density assuming boost invariant • εBj τ > 1 GeV/(fm2 c) in central 7.7 GeV collisions
• From lattice, critical εc=0.34 ± 0.16 GeV/fm3 : central lowest energy 7.7 GeV might be above transition region. A. Bazavov et al. (hotQCD) ,Phys. Rev. D90 (2014) 094503
arXiv: 1509.06727
QGP turn off: jet quenching
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pT range 3.0-3.5 GeV/c Nbin scaled particle yields as a function of Npart
Interplay of Cronin effect, radial flow, coalescence Jet quenching
• At √sNN > 14.5 GeV/c, jet quenching has to be there • At √sNN < 14.5 GeV/c, the jet quenching
feature is gone but we can not rule out jet quenching.
QGP turn off: NCQ scaling and ϕ meson v2
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• NCQ scaling holds for particle and anti-particle separately. • ϕ meson v2, sensitive to QGP, close to zero with large uncertainty at √sNN = 11.5 GeV and below.
QGP turn off: particle and anti-particle v2
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v2 for particle is different from that for anti-particle at lower energies. Hadronic dynamics becomes more and more important at lower energies. Hydro model: Hybrid model (UrQMD + hydro) with baryon stopping Nambu-Jona-Lasinio (NJL): Using vector mean-field potential, repulsive for quarks, attractive for anti-quarks
Hybrid: Phys. Rev. C 86, 044903 (2012) NJL: Acta Phys.Polon.Supp. 7 (2014) 1, 183 Phys. Rev. Lett. 110, 142301 (2013)
Mapping the phase diagram: higher harmonics
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Models show that higher harmonic ripples are sensitive to the presence of a QGP: v3 goes away when the QGP goes away
In more central collisions, v3 is present at the lowest energies, but disappears at lower energies for Npart<50 (turn-off of QGP)
Non-QGP Model 10 210 310
0.04
0.06
0.08
0.1
0.12
0.14
3!10"
ch,PP/n{2}23v
(GeV)NNs
0-5% 10-20% 30-40% 50-60%
When scaled by entropy density, v3 shows a minimum near 15 GeV consistent with an increased bulk viscosity and decreased effective pressure
0 100 200 300
0
0.02
0.04
0.06
0.08
0.1
AMPT Default; 7.7 GeV
{2}23vpartN
partN
=200 GeVNN
s 62.4 39 27 19.6 14.5 11.5 7.7
STAR Collaboration, Phys. Rev. Lett. 116, 112302
Non-QGP Model
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Softening of EOS: v1 slope
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v1 slope: Proton (baryon stopping + pair production) is different from anti-proton (pair production). So is the Lambda. Non-monotonic behavior seen in net-proton v1 slope as a function of collision energy. First order phase transition? softening of EOS? but not for net-kaon.
Softening of EOS: transverse mass or energy
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Particle <mT>-m0 and transverse energy per particle show a flat pattern above ~8 GeV and then increase again Indication of 1st order phase transition ?
0.1
0.2
0.3
0.4
0.5(a) Pions
/+ /-
STAR Preliminary
0.1
0.2
0.3
0.4
0.5(b) Kaons
K+ K-
STAR Preliminary
0
0.25
0.5
0.75
1
1.25 (c) Hadrons
Collision Energy 3sNN (GeV)
Transverse Dynamics in High-Energy Nuclear Collisions
dET/
dd/d
Nch
/dd
(GeV
)<
mT >
- mas
s (G
eV)
1 10 100 1000 10000
ALICE STARPHENIX WA98NA49 E802FOPI
Φmeson
L. van Hove, PLB 118, 138 (1982).
NA49: Phys. Rev. C 78, 4 (2008), Physics Lett. B 491, 59 (2000). STAR: Phys. Rev. C 49, 064903 (2009). ALICE: Phys. Rev. C91, 024609 (2015). M. Nasim et al., Advances in High Energy Physics, 197930 (2015).
Critical point: moments of net charge and net-kaon distributions
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-2
0
2
< 1.6 (GeV/c), |y| < 0.5T
0.2 < p
Au+Au CollisionsNet-Kaon
78 10 20 30 40 100 200-20
-10
0
10
| < 0.5M < 2 (GeV/c), | T
0.2 < p
Net-Charge
STAR 0-5% STAR 70-80% UrQMD 0-5%
Poisson
(GeV)NNs
2 XP
• Net-kaon and net-charge kσ2 are consistent with unity .
• More statistics are needed to draw a conclusion.
• UrQMD without critical point, shows no energy dependence.
Moments of net proton distributions
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2m g
0
1
2
3
4 Range (GeV/c)
Tp
<0.8 T
0.4<p
<1.2T
0.4<p<1.4
T0.4<p
<1.6T
0.4<p< 2
T0.4<p
(STAR: PRL112)
|y|<0.5
Rapidity Range|y|<0.1|y|<0.3|y|<0.4|y|<0.5
<2(GeV/c)T
0.4<p
6 10 20 100 200
)/Ske
llam
m(S
0.6
0.8
1
Net-proton6 10 20 100 200
STAR Preliminary
(GeV)NNsColliding Energy
0-5% Au+Au Central Collisions at RHIC
Results sensitive to kinematic cuts (pT range and rapidity range). With Large acceptance, non-monotonic behavior is seen as a function of √sNN.
Moments of net proton distributions as a function of √sNN
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Non-monotonic trend is observed in central 0-5% collisions
UrQMD without critical point can not explain data, decreases towards lower energy, consistent with baryon number conservation.
X. Luo CPOD2014
(GeV)NNs6 10 20 100 200
2σ
κ
0
1
2
3
4 <2 (GeV/c),|y|<0.5T
0.4<p
0-5%5-10%70-80%
Net-Proton
UrQMD, 0-5%
STAR Preliminary
Au+Au : 0-5%
Net-proton
<2 (GeV/c),|y|<0.5T
0.4<p
STAR data
AMPT
UrQMD
HBT radii: finite-size scaling
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R.Lacey, PRL114,142301(2015)
R2out-R2
side sensitive to the emission duration, shows a non-monotonic trend as a function of collision energy Finite-size scaling analysis indicates a second order phase transition with Tcep ~165 MeV and µcep
B ~ 95 MeV for the location of the critical end point.
What has been achieved from BES I
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QGP turn off signatures • jet quenching feature is gone for Nbin scaled particle yields as a function of Npart at
√sNN < 14.5 GeV. • ϕ meson v2 ~ 0 at √sNN=11.5 and 7.7 GeV with large uncertainties. • Higher harmonics v3 ~ 0 at Npart < 50 at 7.7 GeV.
First order phase transition • When scaled by entropy density, v3 shows a minimum near 15 GeV consistent with
an increased bulk viscosity and decreased effective pressure. • Non-monotonic behavior seen in net-proton v1 slope as a function of √sNN. • Particle <mT>-m0 and transverse energy per particle show a flat pattern At √sNN >
8 GeV and increases again. Critical point: • Non-monotonic trend is seen in moments of net proton distributions in central Au+Au
as a function of collision energy • Non-monotonic trend is seen in the HBT radii as a function of collision energy
Towards BES II
In 2019 & 2020
7.7, 9.1, 11.5, 14.5 and 19.6 GeV
µB from 205 to 420 MeV
10~25 times more statistics
Detector upgrade
- inner Time Projection Chamber
- Event Plane Detector
- endcap Time-Of-Flight
Low Energy Electron Cooling at RHIC
Collision Energies (GeV)
Proposed Event Goals (M)
BES I Event (M)
7.7 100 4
9.1 160 N/A
11.5 230 12
14.5 300 20
19.6 400 36
STAR Note 598
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Upgrade plan for BES II
iTPC upgrade EPD upgrade eTOF upgrade
Continuous pad rows Replace all inner TPC sectors
Replace Beam Beam Counter Add CBM TOF modules and electronics (FAIR Phase 0)
|η|<1.5 2.1<|η|<5.1 -1.6<η<-1.1
pT >60 MeV/c Better trigger & b/g reduction Extend forward PID capability
Better dE/dx resolution Better momentum resolution
Greatly improved Event Plane info (esp. 1st-order EP)
Allows higher energy range of Fixed Target program
Fully operational in 2019 Fully operational in 2018 Fully operational in 2019
endcap Time-Of-Flight
Event Plane Detector
inner Time Projection Chamber
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Net-proton cumulants in BES II with iTPC
Net-proton cumulants revealed a non-trivial energy dependence from BES I. Measure as a function of Δyp in a wide range is needed to establish true nature of correlation iTPC upgrade will enable this measurement in a wider range
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Fixed target program
Fixed target program proposed during RHIC BES II will extend the energy down to √sNN = 3.0 GeV (µB = 721 MeV) The fixed target is outside the STAR TPC at 210 cm Only single beam is used √sNN = 3.0 ~ 7.7 GeV ~100M events needed per energy
Reconstructed 3.9 GeV Au+Au event
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STAR preliminary
Spectra and flow from fixed target
Dedicated fixed-target run in 2015: √sNN = 4.5 GeV • 1 M events in 30 minutes! • Excellent PID using dE/dx and ToF • dN/dy and v1 for charged particles and V0s are in good agreement with published results
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Summary
Many interesting features have been observed for the signatures of • QGP turn off • First-order phase transition • Critical point Turn the qualitative features to quantitative understandings. • exciting results from the future BESII
program • BEST Theory Collaboration
(GeV)NNs4 5 6 7 8 10 20 30 40 100 200
)3/c2
(GeV
2B3−10
E864(d) Au+PbE866(d) Au+AuE877(d) Au+AuNA49(d) Pb+PbPHENIX(d) Au+Au
) Au+AudSTAR() Au+AudPHENIX(
/ A = 0.65 GeV/cT
pSTAR 0-10%(d) Au+Au
) Au+AudSTAR 0-10%(
Average of p+p and p+A
Central CollisionSTAR Preliminary
Light nucleus production at BES I
The coalescence parameter B2 is decreasing with energy and flattening out at about 20 GeV à change in EOS?
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Beam Energy Scan II in 2019-2020
RHIC is unique to study chiral symmetry restoration: Beam energy scan II: collision energies 7.7, 9.1, 11.5, 14.5, 19.6 GeV. Electron cooling from CAD will increase collision rate from 3-10.
Physics impact for the detector upgrade in BES II
Low Energy Electron Cooling at RHIC: Electron Cooling can raise the luminosity by a factor of 3-10 in the range from 5 – 20 GeV Long Bunches increase luminosity by factor of 2-5
The upgrade for BES II will improve many of the STAR analyses Better statistics Better resolution Smaller systematic uncertainty Wider rapidity range Wider pT coverage
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