heavy ion café, univ. of tokyo (dec. 6, 2008) t.chujo proving quark gluon plasma via baryon...
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![Page 1: Heavy Ion Café, Univ. of Tokyo (Dec. 6, 2008) T.Chujo Proving Quark Gluon Plasma via Baryon Production at RHIC Tatsuya Chujo University of Tsukuba](https://reader035.vdocuments.net/reader035/viewer/2022062422/56649ef25503460f94c0356d/html5/thumbnails/1.jpg)
Heavy Ion Café, Univ. of Tokyo (Dec. 6, 2008) T.Chujo
Proving Quark Gluon Plasma via Baryon Production at RHIC
Tatsuya ChujoUniversity of Tsukuba
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Heavy Ion Café, Univ. of Tokyo (Dec. 6, 2008) T. Chujo
Outline
1. Introduction
2. Overview of bulk properties at RHIC
3. Systematic study of baryon enhancement
4. What’s the origin of baryon enhancement?
5. Exploring the QCD phase diagram at RHIC
6. Summary
1. Introduction
2. Overview of bulk properties at RHIC
3. Systematic study of baryon enhancement
4. What’s the origin of baryon enhancement?
5. Exploring the QCD phase diagram at RHIC
6. Summary
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Heavy Ion Café, Univ. of Tokyo (Dec. 6, 2008) T. Chujo
1. INTRODUCTION
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Heavy Ion Café, Univ. of Tokyo (Dec. 6, 2008) T. Chujo
Why baryons* ?(* protons and antiprotons in this talk)
• Heavier mass than the light mesons, sensitive to the collective phenomena, such as a radial flow.
• Sensitive to the baryo-chemical property of the matter.
• Different number of constituent quarks from that for mesons, test of recombination models.
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Heavy Ion Café, Univ. of Tokyo (Dec. 6, 2008) T. Chujo
A lots of data and publications on baryons from RHIC experiments; 1
(spectra, yields, and jet correlations)
• BRAHMS– Nuclear Stopping in Au+Au Collisions at √sNN = 200 GeV, PRL 93, 102301 (2004).
• PHENIX– Scaling Properties of Proton and Antiproton Production in √sNN = 200 GeV Au Au Collisions, PRL 91,
172301 (2003). [TC]
– Identified charged particle spectra and yields in Au+Au collisions at √sNN=200 GeV, PRC 69, 034909 (2004). [TC]
– Nuclear effects on hadron production in d + Au collisions at √sNN = 200 GeV revealed by comparison with p + p data, PRC 74, 024904 (2006). [(TC)]
– Jet structure of baryon excess in Au+Au collisions at √sNN =200 GeV, PRC 71, 051902 (R) (2005).
– Particle-Species Dependent Modification of Jet-Induced Correlations in Au+Au Collisions at √sNN =200 GeV, PRL 101, 082301 (2008).
– Correlated production of p and pbar in Au+ Au collisions at √sNN = 200 GeV, PLB 649 (2007) 359-369.
– Au+Au 62.4 GeV (preliminary) [TC], Cu+Cu 200 GeV (preliminary),– Cu+Cu 22.5, 62.4 GeV (preliminary) [TC], p+p 62.4 GeV (preliminary) [TC]– p+p 200 GeV (new data)
* note: not the complete list.
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to be published before QM09
(hopefully)
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A lots of data and publications on baryons from RHIC experiments; 2
(spectra, yields, and jet correlations)
• PHOBOS– Identified hadron transverse momentum spectra in Au+Au collisions at √sNN = 62.4
GeV, PRC 75, 024910 (2007).
• STAR– Identified Baryon and Meson Distributions at Large Transverse Momenta from Au+Au
Collisions at √sNN = 200 GeV, PRL 97, 152301 (2006).
– Energy dependence of ±, p and p-bar transverse momentum spectra for Au+Au collisions at √sNN = 62.4 and 200 GeV, arXiv:nucl-ex/0703040.
– Identified hadron spectra at large transverse momentum in p + p and d + Au collisions at √sNN = 200 GeV, PLB 637 (2006) 161-169.
– Systematic Measurements of Identified Particle Spectra in pp, d+Au and Au+Au Collisions from STAR, arXiv:0808.2041.
* note: not the complete list.
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Heavy Ion Café, Univ. of Tokyo (Dec. 6, 2008) T. Chujo
A recent STAR publication (systematic study of PID spectra in p+p (200 GeV), d+Au (200 GeV),
Au+Au (62, 130, 200 GeV), arXiv:0808.2041) , K±, p, pbar pT spectra (low pT region only, dE/dx by TPC).
• A nice full paper (60 pages)!
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2. BULK PROPERTIES AT RHIC
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What are the bulk properties (EOS)?• Energy density ()• Temperature (T):
– critical temperature (Tc), initial temperature (Tini), chemical freeze-out temperature (Tch), kinetic freeze-out temperature (Tkin)
• Chemical potential ():
– baryon chemical potential (B), strangeness chemical potential (s), strangeness suppression factor (s)
• Collective flow velocity (<T>)
• Pressure gradient (P), particle emission anisotropy (v2)
• Particle multiplicity (dN/dy, N)
• Transverse energy (dET/dy, ET)
• Transverse momentum distribution (Ed3N/dp3)• Particle abundance and ratio
• Average transverse momentum (<pT>)
• HBT radii (Rout, Rside, Rlong, )
• Velocity of sound (vs)
• Shear viscosity – entropy ratio (/s)
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What are the bulk properties (EOS)?• Energy density ()• Temperature (T):
– critical temperature (Tc), initial temperature (Tini), chemical freeze-out temperature (Tch), kinetic freeze-out temperature (Tkin)
• Chemical potential ():
– baryon chemical potential (B), strangeness chemical potential (s), strangeness suppression factor (s)
• Collective flow velocity (<T>)
• Pressure gradient (P), particle emission anisotropy (v2)
• Particle multiplicity (dN/dy, N)
• Transverse energy (dET/dy, ET)
• Transverse momentum distribution (Ed3N/dp3)• Particle abundance and ratio
• Average transverse momentum (<pT>)
• HBT radii (Rout, Rside, Rlong, )
• Velocity of sound (vs)
• Shear viscosity – entropy ratio (/s)
….10
• red: directly measured by pT spectra• pink: indirectly measured by pT spectra
How the bulk properties change as a function ofcentrality, system and beam energy?
How the bulk properties change as a function ofcentrality, system and beam energy?
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Charged particle multiplicity at RHIC
Cu+CuPreliminary
3-6%, Npart = 100
Au+Au35-40%, Npart = 99
PHOBOS
• Same number of participants, ~same number of charged particle density at RHIC.
• Focus at the mid-rapidity to study the multiplicity scaling of bulk properties.
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Average pT vs. Nch
<pT> scales with √((dN/dy)/S), p+p 200 GeV, Au+Au 62.4, 130, 200 GeV data. Suggests that the kinetic freeze-out properties in Au+Au collisions are energy independent. CGC (gluon saturation): small x gluons overlap and recombine, reducing the total number
of gluons and increasing their transverse energy. Predicts a lower particle multiplicity and larger <pT>. In CGC, <pT> scales with √((dN/dy)/S). Data is consistent with CGC picture.
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factor ~2
factor ~2
ST: Transverse overlap area [fm2]
STAR, arXiv:0808.2041
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Antiparticle-to-Particle Ratios vs. Nch
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pbar/p: • A slight decrease with centrality (130, 200 GeV)• Considerable drop with centrality (62 GeV)
indicating that larger baryon stopping in central collisions.
STAR, arXiv:0808.2041
-/+: Flat and unity.
STAR, arXiv:0808.2041
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PHENIX 62.4 GeV Au+Au
Hum… pbar/p ratio: seems
decreasing with Npart in PHENIX data too.
DNP2004 (TC)
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Bulk properties vs. Nch (1)
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Tch, Tkin <T>
Tch: constant with dNch/dy.close to the lattice QCD: Tc ~160 MeV.universality at RHIC energies.
Tkin: decreasing with dNch/dy.same trend for all systems at RHIC (with dNch/dy)indicating strong expansion and cooling?
STAR, arXiv:0808.2041 STAR, arXiv:0808.2041
<>: incleasing with dNch/dy.
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Bulk properties vs. Nch (2)
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B,s s
B: finite value, weak centrality dependence (baryon stopping at central)
s: close to zero.
• s: approaching to unity with dNch/dy.
Strangeness production is strongly suppressed in p+p, dAu, peripheral Au+Au. In central Au+Au, implying that strangeness is as equally equilibrated as light quarks.
STAR, arXiv:0808.2041 STAR, arXiv:0808.2041
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Bulk properties vs. Nch (3)
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PHENIX
A. Enokizono
HBT v2/
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Bulk properties vs. Nch (4)
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K-/-
“Only” Nch (or initial energy density) determines the bulk properties at RHIC?
“Only” Nch (or initial energy density) determines the bulk properties at RHIC?
STAR, arXiv:0808.2041
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3. SYSTEMATIC STUDY OF BARYON ENHANCEMENT
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Baryon enhancement at RHICPHENIX: PRL 91, 172301 (2003), PRC 69, 034909 (2004), PRC 74, 024904 (2006)
In Au+Au sNN = 200 GeV central collisions:• RCP (or RAA)
• Pions: Strong suppression of yields above pT ~ 2 GeV/c, due to jet quenching.• Protons: No suppression at intermediate pT (2-5 GeV/c).
• p/ and pbar/ ratios• Factor ~3 more (anti) protons than pions at intermediate pT (2-5 GeV/c). • Strong centrality dependence.
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Systematic study of PID spectra: Au+Au, Cu+Cu, p+p at sNN = 22.5, 62.4, 200 GeV
0 pT spectra in Cu+Cu 22.5 GeV
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p+p 62.4 GeV, set the baseline for HI data.PHENIX data agrees
with ISR data.
* No weak decay feed-down correction applied.
s dep. of pbar/- ratio (central)
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Cu+Cu 22.5 GeV, pbar/ ratio in central
agrees with p+p.
s dep. of pbar/- ratio (central)
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Cu+Cu 62.4 GeV, pbar/ ratio larger
than those in p+p and Cu+Cu 22.5 GeV.
s dep. of pbar/- ratio (central)
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Cu+Cu 200 GeV, similar to those in Cu+Cu 62.4 GeV.
s dep. of pbar/- ratio (central)
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Au+Au 62 GeV, pbar/- is
unchanged from Cu+Cu 200 GeV
s dep. of pbar/- ratio (central)
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Au+Au 200 GeV, p-bar/- is enhanced.
s dep. of pbar/- ratio (central)
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Peripheral collisions for all systems
Conversing to the same line
s dep. of pbar/- ratio (peripheral)
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* No weak decay feed-down correction applied.
• In 22.5 GeV Cu+Cu: weak centrality dependence, pbar/- ratios are ~0.3-0.4 at pT = 2 GeV/c, which is close to the value in p+p.• In 62.4 GeV Cu+Cu:pbar/- ratio in central collisions reaches R=~0.6 at pT = 2 GeV/c, decreasing towards the peripheral events.
Centrality dep. of pbar/- (22 GeV vs. 62 GeV)
0.3
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0 1.0 2.0 3.0 pT (GeV/c)
Comparison with SPS data
0.25 Pb+Pb 17.2 GeV (central)
T. Schuster, A. Laszlo (NA49)nucl-ex/0606005
SPS Pb+Pb: consistent with Cu+Cu 22.5 GeV pbar/.
(Au+Au 200 GeV)
(Au+Au 200 GeV)
(Pb+Pb 17.2 GeV)
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• Increasing as a function of s.
• Indicates the onset of baryon enhancement is in between 22 GeV and 62 GeV.
* No weak decay feed-down correction applied.
pbar/- ratio (central): summary
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0 pT spectra in Cu+Cu and p+p at 22.4, 62.4, 200 GeV
PHENIX: PRL 101, 162301 (2008)
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0 RAA in Cu+Cu: energy dep.
• Enhancement at 22 GeV.• Consistent with no energy loss model.
PHENIX: PRL 101, 162301 (2008)
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4. WHAT’S THE ORIGIN OF BARYON ENHANCEMENT?
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Jet induced baryon enhancement?
Near sideAway side
Away side two peaks (shoulder)
Sonic shock wave?Baryon/Meson effect?
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Jet-pair distribution for associated M/B
• Trigger particle: charged hadron (2.5 <pT,trig < 4.0 GeV/c)
• Associate particle: meson or baryons (1.0 – 2.0 GeV/c).
• Near side: substantially weaker for associated baryons.
• Away side: similar for associated mesons and baryons. “Shoulder” structure appeared.
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PHENIX: PRL 101, 082301 (2008)
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Conditional jet yields for M/B• Mesons:
– exponential decrease with increasing pT, assoc.
– Yield increase from peripheral to central, with different slope
– Incompatible with in-vacuum fragmentation
– Due to contribution from correlated soft partons, softening of FF, recombination, energy loss, etc… ?
• Baryons:– different strongly from those for
mesons.
– Not exponential shape.
– Yield (away) > Yield (near).
– Much stronger increase with centrality than those for mesons.
– Might be due to the correlated soft parton recombination.
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PHENIX: PRL 101, 082301 (2008)
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Baryon/meson ratios associated with high pT hadron trigger (2.5 < pT < 4GeV/c)
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• Peripheral ratios ~ vacuum fragmentation• In-jet ratios ~ inclusive p/(+K)
Away-side “shoulder”, and baryon enhancement in single spectra: might be the common origin.
* Recombination of correlated soft partons induced via strong parton medium interactions?
PHENIX: PRL 101, 082301 (2008)
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Au+Au 0-10%STAR preliminary
3 < pt,trig< 4 GeV/cpt,assoc. > 2 GeV/c
Intermediate pT ridge & Jet (near side only) (from SQM08, O. Barannikova, STAR)
pTtrig > 4.0 GeV/c
2.0 < pTAssoc
< pTtrig
p+
p /
++-
Au+Au: 2 < pTtrig < 3 GeV/c
Cu+Cu: 3 < pTtrig < 6 GeV/c
• Jet+ridge yields follow similar trend in pT for all trigger types
(left bottom)
• Production mechanisms for jet and ridge are different (p/,
/K)
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5. EXPLORING THE QCD PHASE DIAGRAM AT RHIC
40
Figure from “Future Science at theRelativistic heavy ion Collider (Aug. 25, 2006 version)”,by RHIC II Science Working Groups
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Excitation functions of freeze-out properties
41
• μB: falls monotonically.
• Tch: rapidly rises at SIS and AGS energy, saturates at SPS and RHIC energies (a unique Tch ~ Tc from lattice QCD).
• Tkin: decoupled at √sNN~10 GeV from Tch. Due to the strong collective flow, matter is cooled prolong period of chemical freeze-out and kinetic freeze-out.
• <> : rapid increase from SIS to AGS, increasing slowly from SPS to RHIC.
Q: Freeze-out properties changes from AGS to SPS (e.g. √sNN~10 GeV )?
Q: Freeze-out properties changes from AGS to SPS (e.g. √sNN~10 GeV )?
STAR, arXiv:0808.2041
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“hone” at SPS is true? K−/π− ratio : steadily increases
with √sNN,while K+/π+ sharply increases at low energies.
A maximum K+/π+ value is reached at about √sNN ≈ 10 GeV.
K+/K- vs sqrt(s): smooth decrease (log scale).
using the functional forms for K+/K- and K-/-, then make the function for K+/+.
• Generates a maximum at 10 GeV (“horn”)..
More detail energy scan is needed.
42
STAR, arXiv:0808.2041
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Yet another onset at RHIC
Cu+Cu
Au+Au
Emergence of opacity
Approach to constant v2
and hydrodynamic limit?
PHENIX: PRL 101, 162301 (2008)
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Onset of Quark Number Scaling?Onset of Quark Number Scaling?
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• Increasing as a function of s.
• Indicates the onset of baryon
enhancement is in between 22 GeV
and 62 GeV.
* No weak decay feed-down correction applied.
p-bar/- ratio vs. √sNN
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Search for QCD Critical Point (QCP)
From C. Nonaka (JPS2008 fall)
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47
From C. Nonaka (JPS2008 fall)
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48
From C. Nonaka (JPS2008 fall)
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49Observable: look at pbar/p vs. pT.
From C. Nonaka (JPS2008 fall)
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6. Summary
• Baryons (protons and antiprotons) has a unique role to characterize the many bulk properties of matter, hadronization mechanism, and medium response.
• Bulk properties at RHIC (at mid-rapidity) : governed by the charged particle multiplicity
– Relevant to the CGC gluon saturation picture.
• Systematic study of baryon enhancement:– qualitative difference between 22 GeV and 62.4 GeV on the
property of baryon enhancement (while freeze-out properties seems to be already changed at 10 GeV).
– Jet correlation: indicating the jet induced baryon enhancement.
• Towards the understanding of QCD phase diagram and QCP search.
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Backup Slides
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sNN dep. of p/+ ratio (central)
• decreasing as a function of s.
* No weak decay feed-down correction applied.
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0 RAA vs. sNN
D. d’Enterria, nucl-ex/0504001
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STAR p+p 200 GeV data (xT scaling)
55
STAR: PLB 637 (2006) 161-169
• In p+p collisions, xT (=2pT/s) scaling works for both inclusive charged hadrons and identified hadrons (pions, protons, and antiprotons).
• Invariant cross sections can be expressed as the following equation:
• The power “n” = 6.3-6.5 showed a good scaling in p+p collisions (c.f. PPG023).
• Indicates soft and hard transition by data.
€
Ed3σ
dp3=
1
sn(xT , s )
G(xT )
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sNN dep. RAA for antiprotons (by ISR fit)
• Used ISR data at 23 GeV and 63 GeV (Alper. NPB 100, 237) for p+p reference.
• Similar RAA for all three systems.
* Note: p+p 62.4 GeV p+p data has been measured by PHENIX, still working on the trigger bias and cross section seen in the detector. Here we use ISR fit to obtain RAA.
* No weak decay feed-down correction applied.
Nuclear Modification Factor
( ) ( )
( )coll
AA T
yield AuAu NR p
yield pp=
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sNN dep. RAA for charged pions (by ISR fit)
Error notations:- Error bars: statistical error for HI spectra- Boxes:
1) sys. error for p+p reference.2) sys. error for HI spectra.
- Lines: Ncoll error (1.)
• Used ISR fit (nucl-ex/0411049, D. d’Enteria) for p+p parameterization.
• Moderate suppression for Au+Au 62.4 GeV.
• Greater than unity for Cu+Cu 62/22 GeV (pT > 2.0 GeV/c).
* No weak decay feed-down correction applied.