strangeness (and heavy flavor) at rhic recent results from phenix
DESCRIPTION
Strangeness (and heavy flavor) at RHIC. Strangeness (and heavy flavor) at RHIC Recent Results from PHENIX. Recent Results from PHENIX. Masashi Kaneta RIKEN-BNL Research Center for the PHENIX collaboration. Masashi Kaneta RIKEN-BNL Research Center. Outlook of this talk. - PowerPoint PPT PresentationTRANSCRIPT
Masashi Kaneta, RIKEN-BNL Research Center, “Strangeness at RHIC : Recent Results from PHENIX”
1
Recent Resultsfrom PHENIX
Masashi Kaneta RIKEN-BNL Research Center
Masashi Kaneta RIKEN-BNL Research Centerfor the PHENIX collaboration
Strangeness (and heavy flavor) at RHIC
Recent Resultsfrom PHENIX
Strangeness (and heavy flavor) at RHIC
Masashi Kaneta, RIKEN-BNL Research Center, “Strangeness at RHIC : Recent Results from PHENIX”
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Outlook of this talkOutlook of this talk
• PHENIX experiment
• Future strangeness and heavy flavor measurement at PHENIX– Charged hadron identification at high pT: Aerogel Cherenkov Counter
– Upgrade around vertex : Silicon Vertex, Hadron Blind Detector, TPCNosecone Calorimeter
• Recent results from PHENIX– Event anisotropy
• 62.4GeV Au+Au : , K, p, and p (comparing with 200GeV)• 200 GeV Au+Au : Heavy flavor electron
– Single particle spectra of • 200GeV d+Au and 200GeV Au+Au
– Anti-Pentaquark search and capability of the other strangeness• 200GeV p+p, d+Au, and Au+Au
– Heavy Flavor Results from PHENIX• See talk of H. Pereira (Saclay) on Sep. 17 (Fri)
• Summary
Masashi Kaneta, RIKEN-BNL Research Center, “Strangeness at RHIC : Recent Results from PHENIX”
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USA Abilene Christian University, Abilene, TXBrookhaven National Laboratory, Upton, NYUniversity of California - Riverside, Riverside, CAUniversity of Colorado, Boulder, COColumbia University, Nevis Laboratories, Irvington, NYFlorida State University, Tallahassee, FLFlorida Technical University, Melbourne, FLGeorgia State University, Atlanta, GAUniversity of Illinois Urbana Champaign, Urbana-Champaign, ILIowa State University and Ames Laboratory, Ames, IALos Alamos National Laboratory, Los Alamos, NMLawrence Livermore National Laboratory, Livermore, CaUniversity of New Mexico, Albuquerque, NMNew Mexico State University, Las Cruces, NMDept. of Chemistry, Stony Brook Univ., Stony Brook, NYDept. Phys. and Astronomy, Stony Brook Univ., Stony Brook, NY Oak Ridge National Laboratory, Oak Ridge, TNUniversity of Tennessee, Knoxville, TNVanderbilt University, Nashville, TN
Brazil University of São Paulo, São PauloChina Academia Sinica, Taipei, Taiwan
China Institute of Atomic Energy, BeijingPeking University, Beijing
France LPC, University de Clermont-Ferrand, Clermont-FerrandDapnia, CEA Saclay, Gif-sur-YvetteIPN-Orsay, Universite Paris Sud, CNRS-IN2P3, OrsayLLR, Ecòle Polytechnique, CNRS-IN2P3, PalaiseauSUBATECH, Ecòle des Mines at Nantes, Nantes
Germany University of Münster, MünsterHungary Central Research Institute for Physics (KFKI), Budapest
Debrecen University, DebrecenEötvös Loránd University (ELTE), Budapest
India Banaras Hindu University, BanarasBhabha Atomic Research Centre, Bombay
Israel Weizmann Institute, RehovotJapan Center for Nuclear Study, University of Tokyo, Tokyo
Hiroshima University, Higashi-HiroshimaKEK, Institute for High Energy Physics, TsukubaKyoto University, KyotoNagasaki Institute of Applied Science, NagasakiRIKEN, Institute for Physical and Chemical Research, WakoRIKEN-BNL Research Center, Upton, NYRikkyo University, TokyoTokyo Institute of Technology, TokyoUniversity of Tsukuba, TsukubaWaseda University, Tokyo
S. Korea Cyclotron Application Laboratory, KAERI, SeoulKangnung National University, KangnungKorea University, SeoulMyong Ji University, Yongin CitySystem Electronics Laboratory, Seoul Nat. University, SeoulYonsei University, Seoul
Russia Institute of High Energy Physics, ProtovinoJoint Institute for Nuclear Research, DubnaKurchatov Institute, MoscowPNPI, St. Petersburg Nuclear Physics Institute, St. PetersburgSt. Petersburg State Technical University, St. Petersburg
Sweden Lund University, Lund
12 Countries; 58 Institutions; 480 Participants*
*as of January 2004
Masashi Kaneta, RIKEN-BNL Research Center, “Strangeness at RHIC : Recent Results from PHENIX”
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PHENIXPHENIX• Collision vertex and centrality
– Beam-Beam Counters (BBC)– Zero Degree Calorimeters (ZDC)
• Tracking of Charged particle– Drift Chambers (DC)– Pad Chambers (PC1, PC2, PC3)
• , K, p, d, ... ID by Time-Of-Flight– Start timing from BBC– Stop timing from
High resolution TOF detectors (TOF)TOF from Lead Scintillator EMCal (PbSc)
• Electron ID– Ring Image Cherenkov (RICH) detectors– EMCal (PbSc, PbGl)
• Photon (0, , ...)– EMCal (PbSc, PbGl)
• Muon– Muon Tracker (MuTr)
Cathode-strip readout chamber
– Muon Identifier (MuID)Streamer (Iarocci) tube and steel
Masashi Kaneta, RIKEN-BNL Research Center, “Strangeness at RHIC : Recent Results from PHENIX”
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Publication about Strangeness and Heavy Publication about Strangeness and Heavy FlavorFlavor
• Single Identified Hadron Spectra from sNN = 130 GeV Au+Au Collisions– K. Adcox et al., Phys. Rev. C 69, 024904 (2004)
• Centrality dependence of , K, p andp production from sNN =130 GeV Au+Au collisions
at RHIC– K. Adcox et al., Phys. Rev. Lett. 88, 242301 (2002)
• Measurement of the and particles in Au+Au Collisions at sNN =130 GeV– K. Adcox et al., Phys. Rev. Lett. 89, 092302 (2002)
• Identified Charged Particle Spectra and Yields in Au+Au Collisions at sNN = 200 GeV – S. S. Adler et al., Phys. Rev. C 69, 034909 (2004)
• Elliptic Flow of Identified Hadrons in Au+Au Collisions at sNN = 200 GeV– S.S. Adler et al, Phys.Rev.Lett. 91 182301 (2003)
• Measurement of Single Electrons and Implications for Charm Production in Au+Au Collisions
at sNN =130 GeV– K. Adcox et al., Phys. Rev. Lett. 88, 192303 (2002)
• J/ production from proton-proton collisions at s = 200 GeV– S.S. Adler et al., Phys. Rev. Lett. 92, 051802 (2004)
• J/ Production in Au-Au Collisions at sNN =200 GeV at the Relativistic Heavy Ion Collider– S.S. Adler et al., Phys. Rev. C 69, 014901 (2004)
Masashi Kaneta, RIKEN-BNL Research Center, “Strangeness at RHIC : Recent Results from PHENIX”
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Bulk Properties at RHIC Bulk Properties at RHIC
• What we learnt from RHIC?– Low pT (<~2GeV/c) phenomena
• Thermalization– Elliptic Flow
» Agreement with Hydrodynamical calculations– Chemical freeze-out
» The model well describes the data and strangeness equilibration at RHIC– Radial Flow
» Single spectra of , K, p are described by common temperature and flow velocity
– Intermediate and high pT (>~2GeV/c) phenomena• Dense matter effect in Au+Au collisions
– High pT suppression in single particle spectra
– Back-to-Back jet suppression
• Different effect in Baryon/meson– Mass scaling?– Due to number of consistent quarks?– Any difference in flavor (between light quark (u,d) and s)?
Topics relatedto this talk
Masashi Kaneta, RIKEN-BNL Research Center, “Strangeness at RHIC : Recent Results from PHENIX”
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Elliptic FlowElliptic Flow
Masashi Kaneta, RIKEN-BNL Research Center, “Strangeness at RHIC : Recent Results from PHENIX”
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Elliptic Flow at 62.4 GeV Au+AuElliptic Flow at 62.4 GeV Au+Au
• Identified particle v2 from 62.4 GeV Au+Au– Looks similar , K, p dependence with 200GeV Au+Au– With more statistics, we will be able to do detail analyses
• Centrality dependence• More particle species (How about , etc.?)
v 2
pT [GeV/c]
PHENIX preliminary
sNN = 62.4 GeV Au+Au centrality : 0-84%
stat. error onlysys. error <20%
v 2
pT [GeV/c]
Charged ,K,p : PRL91, 182301 (2003)0 : work in progress
sNN = 200 GeV Au+Au centrality : 0-92%
stat. error onlysys. error <15%
Masashi Kaneta, RIKEN-BNL Research Center, “Strangeness at RHIC : Recent Results from PHENIX”
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Elliptic flow : Elliptic flow : nnquarkquark Scaling Scaling
• A scaling of number of constituent quark– Quark coalescence picture
stat. error onlysys. error <20% (62GeV) 15% (200GeV)
62.4 GeV Au+Au: PHENIX preliminary200 GeV Au+Au, charged p,K,p : from PRL 0 : work in progress
pT /nquark [GeV/c]
v 2 /n
quar
k• 62.4GeV Au+Au– The scaling looks
working like 200 GeV Au+Au
– Seems to be slightly lower than 200 GeV in pT/nquark<1 GeV/c
Masashi Kaneta, RIKEN-BNL Research Center, “Strangeness at RHIC : Recent Results from PHENIX”
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vv22 of Heavy Flavor Electrons of Heavy Flavor Electrons
• v2 of Heavy flavor electron– Looks consistent with/without charm flow– We hope that run4 data will give an answer
0 1 2 3 40 1 2 3 4pT [GeV/c]
0.3
0.25
0.2
0.15
0.1
0.05
0
-0.05
-0.1
v 2
bin width
systematic errors ofestimation
Inclusive e± v2(statistical error only)
Heavy flavor e± v2100% of “photonic electron”
“r (pT)” “ ”
sNN = 200 GeV Au+Au centrality : 0-92%
Photonic electron : e± from• Dalitz decay of 0, , , • di-electron decays , , • photon conversions• kaon decays ( e)
r : photonic electron
/ inclusive electron
Glossary
v2inclusive-e - r v2
photo-electron
1 – r
v2heavy-flavor-e
=
Estimation of v2Heavy Flavore± v2
w/ charm floww/o charm flow
V. Greco, C.M. Ko, R. Rappnucl-th/0312100
Hor. bar : stat. err.
Box : total sys. err.
work in progress
Masashi Kaneta, RIKEN-BNL Research Center, “Strangeness at RHIC : Recent Results from PHENIX”
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mesonmeson
Masashi Kaneta, RIKEN-BNL Research Center, “Strangeness at RHIC : Recent Results from PHENIX”
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measurement at PHENIXmeasurement at PHENIX
• Both K+K- and e+e- channel are available– K : mass square from Time-of-Flight from TOF detector and EMCal– e : RICH and EMCal
Kaon ID : TOF of PbSc EMCal
work in progress
Cou
nts
/ bi
n
S ~ 120S/B = 1/4
Cou
nts
/ bi
n
Invariant mass [GeV/c2] Invariant mass [GeV/c2]
K+K-e+e-
work in progress
Run3 sNN = 200 GeV d+Au
Masashi Kaneta, RIKEN-BNL Research Center, “Strangeness at RHIC : Recent Results from PHENIX”
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Single Particle Spectra of Single Particle Spectra of ]
)[(
GeV
/c
2
12-
22
dydm
Nd
mT
T
0 0.5 1 1.5 2 2.5 3
mT – mass [GeV/c2]
1
10-1
10-2
10-3
10-4
10-5
10
PHENIX final datato be submitted to PRC
sNN = 200 GeV Au+Au
K+K-
mT – mass [GeV/c2]
0 0.5 1 1.5 2 2.5 3
10-1
10-2
10-3
10-4
10-5
PHENIX preliminary
sNN = 200 GeV d+Au, Min. Bias
e+e-
K+K-
Masashi Kaneta, RIKEN-BNL Research Center, “Strangeness at RHIC : Recent Results from PHENIX”
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Inverse Slope Parameter and Yield of Inverse Slope Parameter and Yield of
• Extracting inverse slope parameter and yield– Using a fit function
m)/T(m e
m)TTπ
dN/dy
dydm
Nd
mπT
TT
( 2
2
2
1
Inverseslopeparameter
yield
mT – mass [GeV/c2]
0 0.5 1 1.5 2 2.5 3
10-1
10-2
10-3
10-4
10-5
PHENIX preliminary
sNN = 200 GeV d+Au, Min. Bias
e+e-
K+K-
stat. err. only
])
[(G
eV
/c
2
12-
22
dy
dm
Nd
mT
T
0 0.5 1 1.5 2 2.5 3
mT – mass [GeV/c2]
1
10-1
10-2
10-3
10-4
10-5
10
PHENIX final datato be submitted to PRC
sNN = 200 GeV Au+Au
K+K-
stat. err. only
Masashi Kaneta, RIKEN-BNL Research Center, “Strangeness at RHIC : Recent Results from PHENIX”
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Inverse Slope Parameter and Yield of Inverse Slope Parameter and Yield of
• Inverse slope of – Flat as a function of <Npart>
• Over d+Au and Au+Au• Within statistics +
systematic error
• Yield of – Increasing with <Npart>
– Not simple linear of <Npart>
<Npart>
Inve
rse
Slo
pe P
ara
met
er [
Me
V] 200 GeV d+Au (preliminary)
200 GeV Au+Au w/ centrality cut 200GeV Au+Au Min. Bias
Hor. bar : stat. err.
Box : total sys. err.
0 100 200 300 0 100 200 300
dN/d
y
<Npart> <Npart>
(dN
/dy)
/ (
2<N
pa
rt>
)
200 GeV d+Au (preliminary)
200 GeV Au+Au w/ centrality cut
200GeV Au+Au Min. Bias
Hor. bar : stat. err.
Box : total sys. err.
Masashi Kaneta, RIKEN-BNL Research Center, “Strangeness at RHIC : Recent Results from PHENIX”
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Com
puted by Akio K
iyomichi (2003 D
NP
/ 2004 JPS
meeting)
Radial flowRadial flow
• Single particle spectra of , K, p,p– Well described by Blast wave mode (E.Schnedermann et al, PRC48, 2462 (1993)) fit– Common thermal freeze-out temperature and flow velocity for , K, p,p– How about for phi meson?
Fit range : mT – mass < 1 GeV/c2
Masashi Kaneta, RIKEN-BNL Research Center, “Strangeness at RHIC : Recent Results from PHENIX”
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Does Does has same has same TTfofo and < and <TT> with > with , , KK, , pp ? ?
• Simultaneous fit– The 2 contour plot for each particle
200 GeV Au+Au, 40-92%
• Within 3 – Overlap of with , K, p– Large area of 2 contour for
• Because of larger statistical error (i.e. smaller 2) of than , K, p
• Need more statistics to conclude
Fit rangemT -mass < 1 GeV/c2
, K, p,p
, K, p,p,
200 GeV Au+Au, 10-40%200 GeV Au+Au, top 10%
3 2
1
Masashi Kaneta, RIKEN-BNL Research Center, “Strangeness at RHIC : Recent Results from PHENIX”
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Does Does has same has same TTfofo and < and <TT> with > with , , KK, , pp ? ?
• Simultaneous fit by , K, p,p and – Seems to be common Tfo and <T>
– But don’t hurry up to conclude– Again, need more statistics
Fit range mT -mass < 1 GeV/c2
200GeV Au+Au, K, p : PHENIX, PRC 69, 034909 (2004) : PHENIX final (to be submitted to PRC)
Masashi Kaneta, RIKEN-BNL Research Center, “Strangeness at RHIC : Recent Results from PHENIX”
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Intermediate Intermediate ppTT phenomena phenomena
• Energy loss effect in proton at intermediate pT is different from pion
– Note : Those are expected to be merged at very high pT
(=R
cp)
Y
ield
(0
– 1
0%
) /
Nco
ll(0
– 1
0%
)
Yie
ld (
40
– 9
2%
) /
Nco
ll(4
0 –
92
%)
pT [GeV/c2]
• Rcp of is close to pion rather than proton
– Address a scaling of number of constituent quarks
– Statistical error is still large
• Need more statistic
Shown in PHENIX white paper sNN = 200 GeV Au+Au
Masashi Kaneta, RIKEN-BNL Research Center, “Strangeness at RHIC : Recent Results from PHENIX”
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Exotic Particle Exotic Particle SearchSearch
in RHIC Energyin RHIC Energyat PHENIXat PHENIX
Masashi Kaneta, RIKEN-BNL Research Center, “Strangeness at RHIC : Recent Results from PHENIX”
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Anti-Pentaquark SearchAnti-Pentaquark Search
• Motivation: Why anti-pentaquark?– If a particle exists, anti-particle does– Anti-Baryon to Baryon ratio is high (>~0.7) at RHIC energy
• Channel– K+ +n– PHENIXn measurement is unique at RHIC (so far)
• Large energy deposit in EMCal• Not photon-like shower shape• No charged track association on the candidate• Momentum reconstruction from Time-Of-Flight
Summary table from hep-ex/0406077
• Pentaquark state is still not established yet
– Many positive results– Many negative results
• How about at PHENIX?– So far, negative with current statistics
– We report a summary of the search in
s(NN) =200 GeV p+p, d+Au, Au+Au
Masashi Kaneta, RIKEN-BNL Research Center, “Strangeness at RHIC : Recent Results from PHENIX”
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Reliability of Anti-Reliability of Anti-nn Candidate Candidate
• Anti-n momentum resolution checked
– Applying the reconstruction method to anti-proton
• Comparison of momentum from TOF and tracking
– Resolution<4%,10%,15% in pT<1.0, 1.5, 2.0 GeV/c,
respectively
– Momentum shift <~5%
pT [GeV/c]
mas
s pe
ak [G
eV/c
]
Marker : Data
Dash line : MC
-
+
mas
s fr
om P
DG
– Invariant mass peak of
-(1189.4) n + - : R.R. 99.85%, c-= 2.396cm
+(1197.4) n + + : B.R. 48.31%, c+= 4.434cm
• Mass shift due to no TOF calibration for n in EMCal is <~5%• Quick check by Monte-Carlo shows agreement with data
- +
1.1 1.2 1.3 1.4 1.5 1.6 1.1 1.2 1.3 1.4 1.5 1.6
Cou
nts
/ bin
n + - n + +
No pT cut No pT cut
200 GeV p+p 200 GeV p+p
Same eventhigh pT photon trigger
Mixed eventMinBias trigger
Invariant mass [GeV/c2]
Masashi Kaneta, RIKEN-BNL Research Center, “Strangeness at RHIC : Recent Results from PHENIX”
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K K + + ++nn in in pp ++pp, d+Au, Au+Au, d+Au, Au+Au•Run3 s = 200 GeV p+p
– Minimum bias trigger– 35 M events– 5 MeV/c2 per bin
work-in progressSame event
Mixed event
Cou
nts
/ bin
work in progress
•Run3 sNN = 200 GeV d+Au– Minimum bias trigger– 91 M events– 5 MeV/c2 per bin
Same event
Mixed event
Cou
nts
/ bin
Top 30% central 30-50% 50-92%
work in progress
work in progress
work in progress
Same event
Mixed event
•Run2 sNN = 200GeV Au+Au– Minimum bias trigger
– 36M events– 4 MeV/c2 per bin
Cou
nts
/ bin
No significant signal seen
Masashi Kaneta, RIKEN-BNL Research Center, “Strangeness at RHIC : Recent Results from PHENIX”
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More Strangeness at PHENIXMore Strangeness at PHENIX
• From combinations of ±, K±, p,p, andn
Invariant mass [GeV/c2]
0
K0s pT =1-2 GeV/c
Invariant mass [GeV/c2]
pT =1-2 GeV/c
Invariant mass [GeV/c2]
K*0
pT =1-2 GeV/c
Invariant mass [GeV/c2]
Not enoughstatistics..
pT =1-2 GeV/c
Invariant mass [GeV/c2]
pT =1-2 GeV/c
Invariant mass [GeV/c2]
pT =1-2 GeV/c
Invariant mass [GeV/c2]
pT =1-2 GeV/c
• Demonstration from– Run3 sNN =200 GeV p+p
– ~24M events of Min Bias trigger
• Blue histograms– Pair from save event
• Red histograms– Combinatorial back ground
from event mixing from Min. Bias trigger
– Normalization range» solid filled area
Masashi Kaneta, RIKEN-BNL Research Center, “Strangeness at RHIC : Recent Results from PHENIX”
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Future Measurement Future Measurement of Strangeness of Strangeness
and Heavy Flavorand Heavy Flavorat PHENIXat PHENIX
Masashi Kaneta, RIKEN-BNL Research Center, “Strangeness at RHIC : Recent Results from PHENIX”
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Aerogel Cherenkov CounterAerogel Cherenkov Counter
• Modules for half sector are installed in 2003– Left half modules are already installed in July 2004
• Enhancement of PID capability at PHENIX– Proton separation from /K up to p = 7 GeV/c
chargedtrack
160 segments
z (beam
) dire
ction
Azim
uthal angle
Half of th
em in
2003
Reflector (Goretex) PMT
(3 inch)
Aerogel (index~1.011) ( 11x22x20
cm3 )
Integration Cube (Air)PMT(3 inch)
Masashi Kaneta, RIKEN-BNL Research Center, “Strangeness at RHIC : Recent Results from PHENIX”
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PID Plot with Aerogel Cherenkov PID Plot with Aerogel Cherenkov CounterCounter
• With(without) requiring Cherenkov light associated to the track
– We can see pion enhancement (rejection)
– It will be functional to study intermediate pT range
Aerogel Required (Np.e.>3 in each PMT) Aerogel Veto (Np.e.<1 in each PMT)
Peak position(calibration is not perfect yet)Experimental resolution (2-sigma) line
Statistics used for this analysis is less than 4% of total data from run4
Masashi Kaneta, RIKEN-BNL Research Center, “Strangeness at RHIC : Recent Results from PHENIX”
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Upgrade Plan around VertexUpgrade Plan around Vertex
= 1.17
= 0.88
= 0.70
= 0.35
Provides tracking coverage over -2.6 < < 2.6
• Silicon Vertex detector and TPC– Enhancement of momentum resolution– Measurement of in-flight-decay particle
• Will reduce background at high pT
= 2.6
• Nosecone Calorimeter– Jet measurement in
forward region
• Hadron Blind Detector(not shown in the plot)
– Surrounds TPC– Electron ID by
Cherenkov radiation detected by a photocathode layer
Masashi Kaneta, RIKEN-BNL Research Center, “Strangeness at RHIC : Recent Results from PHENIX”
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SummarSummaryy
Masashi Kaneta, RIKEN-BNL Research Center, “Strangeness at RHIC : Recent Results from PHENIX”
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SummarySummary• Elliptic flow of charged , K, p from 62.4 GeV Au+Au
– Similar , K, p dependence with 200GeV Au+Au
– Quark coalescence picture still works in pT /nquark<1 GeV/c
• Heavy flavor electron from 200 GeV Au+Au– Consistent with/without Charm flow
• Cross section of meson– 200GeV d+Au and Au+Au
• Less <Npart> dependence of inverse slope parameter (from mT exponential fit)
• dN/dy increases with <Npart>, but liner scaling
– Study of blast wave model fit• There is overlap of (Tfo, <T>) of with , K, p
– But large range of within-3-sigma of – need more statistics for detail analysis
– Rcp is close to pion’s• support quark number scaling not mass
• Anti-Pentaquark search at PHENIX– No significant signal in 200 GeV p+p, d+Au, Au+Au
• It might be due to S/N ratio is poor at PHENIX• Because of no significant peak of (1520)
– With mixing-event technique, we will have the other strangeness
• New detectors– Aerogel Cherenkov counters are installed
• PHENIX PID capability (proton separation from /K) will be increased up to pT=7 GeV/c
– Silicon VTX, HBD, TPC will come to help electron measurements
Masashi Kaneta, RIKEN-BNL Research Center, “Strangeness at RHIC : Recent Results from PHENIX”
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About Sound Between SectionsAbout Sound Between Sections
You hear sound between sections. That is from “Noh” which is Japanese traditional lyrical drama. “Noh” is completed as current style about 800 years ago in Muromachi shogunate era. The voice is “Yohhhh.” Following that, the sound of musical instrument “Pon” is hit of “Tsuzumi” which is Japanese hand drum. The voice and sound of Tsuzumi are used for adjustment of timing and atmosphere of a serif, and changing a scene. Therefore, I used it for changing section and subject.
By the way, the opening music is not traditional. I borrowed it from a recent Japanese drama.
Masashi KanetaYoh Pon
Yohhh Po Po Pon
Click them {
Masashi Kaneta, RIKEN-BNL Research Center, “Strangeness at RHIC : Recent Results from PHENIX”
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BackupBackup
Masashi Kaneta, RIKEN-BNL Research Center, “Strangeness at RHIC : Recent Results from PHENIX”
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BBC Reaction Plane ResolutionBBC Reaction Plane Resolution<cos(2[BBCN-BBCS])><sin(2[BBCN-BBCS])>
BBC Charge sum
Cor
rela
tion
Cor
rela
tion
200 GeV Au+Au
62.4 GeV Au+Au
Masashi Kaneta, RIKEN-BNL Research Center, “Strangeness at RHIC : Recent Results from PHENIX”
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1/”r”1/”r”In
clus
ive
elec
tron
/ ph
oton
ic e
lect
ron
Masashi Kaneta, RIKEN-BNL Research Center, “Strangeness at RHIC : Recent Results from PHENIX”
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Heavy flavor electron v2Heavy flavor electron v2
).(2.)(2)(2 pnpnppee vNvNvN
. pnpe NNN {
)(
).(2)(2).(2.)(2
)(2e
pnpepp
e
pnpnpp
e N
vNNvN
N
vNvNv
).(2)(2 1 pne
pp
e
p vN
Nv
N
N
).(2)(2 1 pnp vrvr
inclusive electronphotonic electronnon-photonic (=heavy flavor) electron
Masashi Kaneta, RIKEN-BNL Research Center, “Strangeness at RHIC : Recent Results from PHENIX”
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Anti-Neutron PIDAnti-Neutron PID
1 channel 5.5cm
Ene
rgy
depo
sit/
tow
er [
GeV
]
0.5GeV photon
0.5GeV anti-n
MC
MC Ene
rgy
charge EMC TOF
- +
K- K+
pbar p
all charged tracks Data
Energy depositof absorption
Masashi Kaneta, RIKEN-BNL Research Center, “Strangeness at RHIC : Recent Results from PHENIX”
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PID Capability with ACCPID Capability with ACC
Run4 Au+Au 200GeV
K
TOF Aerogel (+ TOF or RICH) RICH
Momentum[GeV/c]
Kp
1 2 3 4 5 6 70.5 2.5
~104.2
Aerogel : (n=1.011.)TOF : 100 ps time resolutionRICH : CO2, (n = 1.00041)
5.53.7
Masashi Kaneta, RIKEN-BNL Research Center, “Strangeness at RHIC : Recent Results from PHENIX”
38
STAR PHENIXSTAR PHENIX
])
[(G
eV
/c
2
12-
22
dy
dm
Nd
mT
T
0 0.5 1 1.5 2 2.5 3
mT – mass [GeV/c2]
1
10-1
10-2
10-3
10-4
10-5
10
PHENIX final datato be submitted to PRC
sNN = 200 GeV Au+Au
K+K-
STAR 200GeV Au+Au from preprint
Masashi Kaneta, RIKEN-BNL Research Center, “Strangeness at RHIC : Recent Results from PHENIX”
39
STAR PHENIXSTAR PHENIX
0 100 200 300 0 100 200 300
dN/d
y
<Npart> <Npart>
(dN
/dy)
/ (2
<N
part>
)
200 GeV d+Au (preliminary)
200 GeV Au+Au w/ centrality cut
200GeV Au+Au Min. Bias
Hor. bar : stat. err.
Box : total sys. err.
STAR 200GeV Au+Au from preprint
<Npart>
Inve
rse
Slo
pe P
aram
eter
[MeV
]
200 GeV d+Au (preliminary) 200 GeV Au+Au w/ centrality cut 200GeV Au+Au Min. Bias
Hor. bar : stat. err.
Box : total sys. err.
Masashi Kaneta, RIKEN-BNL Research Center, “Strangeness at RHIC : Recent Results from PHENIX”
40
STAR PHENIXSTAR PHENIX
pT<~1 GeV/c