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Recent Results from STAR

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For the STAR Collaboration ... Spatial anisotropy Momemtum anisotropy ... transforms the initial spatial anisotropy into the observed momentum anisotropy ... – PowerPoint PPT presentation

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Title: Recent Results from STAR


1
Recent Results from STAR
14th Topical Conference on Hadron Collider Physics
  • Markus D. Oldenburg

Munich, Germany
For the STAR Collaboration
2
Outline
  • RHIC
  • STAR
  • Analyses
  • Anisotropic Flow
  • Jets at RHIC
  • Ultra-Peripheral Collisions
  • Summary
  • Outlook

3
The Relativistic Heavy Ion Collider
  • Two independent accelerator rings
  • 3.83 km in circumference
  • Accelerates everything from p to Au
  • Running conditions Au-Au 2001
  • 55-56 bunches per ring (tested up
    to 110)
  • 7.5?108 Au/bunch _at_ storage energy
  • Storage energy 100 GeV/A
  • Peak luminosity 5?1026 cm-2 s-1
  • Running conditions p?p? 2001
  • 55 bunches per ring
  • 0.8?1011 p?/bunch
  • Energy/beam 100 GeV
  • Peak luminosity 1.5?1030 cm-2 s-1
  • Beam polarization 25 (? AGS)

Long Island
4
The STAR experiment at RHIC
STAR uses the worlds largest Time Projection
Chamber
5
One of the first Au on Au Events at CM Energy of
200 GeV?A
6
Anisotropic Flow
  • Look at peripheral collisions
  • Overlap region is not symmetric in coordinate
    space
  • Almond shaped overlap region
  • Easier for particles to emerge in the direction
    of x-z plane
  • Larger area shines to the side
  • Spatial anisotropy ? Momemtum anisotropy
  • Interactions among constituents generate a
    pressure which transforms the initial spatial
    anisotropy into the observed momentum anisotropy
  • Perform a Fourier decomposition of the momentum
    space particle distributions in the x-y plane
  • vn is the n-th harmonic Fourier coefficient of
    the distribution of particles with repsect to the
    reaction plane
  • v1 directed flow
  • v2 elliptic flow

7
v2 vs. Centrality (130 GeV)
  • v2 is large
  • 6 in peripheral collisions
  • Smaller for central collisions
  • Hydro calculations are in reasonable agreement
    with the data
  • In contrast to lower collision energies where
    hydro over-predicts anisotropic flow
  • Anisotropic flow is developed by
    rescattering
  • Data suggests early time history
  • Quenched at later times

Anisotropic transverse flow is large at RHIC
8
v2 vs. pt and Particle Mass (130 GeV)
  • The mass dependence is reproduced by hydrodynamic
    models
  • Hydro assumes local thermal equilibrium
  • At early times
  • Followed by hydrodynamic expansion

D. Teaney et al., QM2001 Proc.P. Huovinen et
al., nucl-th/0104020
Hydro does a surprisingly good job
9
v2 for High pt Particles (130 GeV)
  • pQCD inelastic energy loss parameterized hydro
    component (M. Gyulassy, I. Vitev and
    X.N. Wang, PRL 86 (2001) 2537)
  • value of v2 at high pt sensitive to the initial
    gluon density
  • saturation and decrease of v2 as a function of pt
    at higher pt
  • data starts to deviate from hydrodynamics at pt gt
    2 GeV/c

Adler et al., nucl-ex/0206006
Data is in qualitative agreement with
jet-quenching scenario
10
Centrality dependence of v2(pt)
130 GeV
  • v2 is saturated at high pt and it does not come
    back down as rapidly as expected
  • What does v2 do at very high pt ?

200 GeV (preliminary)
11
v2 up to 12 GeV/c
v2 seems to remain saturated
12
Hard Probes in Heavy-Ion Collisions
  • New opportunity using Heavy Ions at RHIC ? Hard
    Parton Scattering
  • ?sNN 200 GeV at RHIC
  • 17 GeV at CERN SPS
  • Jets and mini-jets
  • 30-50 of particle production
  • High pt leading particles
  • Azimuthal correlations
  • Extend into perturbative regime
  • Calculations reliable (?)
  • Scattered partons propagate through matter
  • radiate energy (dE/dx x) in colored medium
  • Interaction of parton with partonic matter
  • Suppression of high pt particles jet quenching
  • Suppression of angular correlations

13
Jets in Hadronic Collisions
AuAu ???? (STAR_at_RHIC)
pp ?jetjet (STAR_at_RHIC)
14
Identifying jets on a statistical basis in Au-Au
STAR Preliminary AuAu _at_ 200 GeV/c, 0-5 most
central 4 lt pt(trig) lt 6 GeV/c, 2 lt pt(assoc.) lt
pt(trig)
  • Given a trigger particle with pt gt pt (trigger),
    associate particles with pt gt pt (associated)
  • AuAu
  • flow
  • pp and AuAu collisions
  • dijets
  • momentum conservation
  • jets
  • resonances

All ??
Small ??
15
Peripheral AuAu data vs. ppflow
  • Ansatz
  • A high pt triggered AuAu event is a
    superposition of a high pt triggered
  • pp event plus anisotropic transverse flow
  • v2 from reaction plane analysis
  • A is fit in non-jet region (0.75 lt ?? lt
    2.24)

16
Central AuAu data vs. ppflow
17
Jets at RHIC
  • The backward going jet is missing in central
    Au-Au collisions when compared to p-p data flow
  • Other features of the data
  • High pt charged hadrons dominated by jet
    fragments
  • Relative charge
  • Azimuthal correlation width
  • Evolution of jet cone azimuthal correlation
    strength with centrality

Surface emission?
  • Other explanations for the disappearance of
    back-to-back correlations in central Au-Au?
  • Investigate nuclear kT effects
  • Experiment pAu or dAu
  • Theory Add realistic nuclear kT to
    the models

?
Suppression of back-to-back correlations in
central AuAu collisions
18
Ultra-Peripheral Collisions
  • b gt 2RA
  • no hadronic interactions
  • ltbgt 20-60 fermi at RHIC
  • Ions are sources of fields
  • Fields couple coherently to ions
  • pt lt h/RA, 30 MeV/c for heavy ions
  • p lt gh/RA 3 GeV/c at RHIC
  • Photonuclear (Photon-Pomeron) Interactions
  • gA r0, w, f, J/y, A
  • Vector Meson Dominance
  • gA qqA (elastic scattering) VA
  • s(r) 350 mb at 130 GeV/nucleon
  • 5 of sAuAu(had.)
  • Electromagnetic particle production
  • gg leptons, mesons
  • Strong Field (nonperturbative?) QED

-
19
Exclusive r0
200GeV
  • Trigger on low multiplicity events
  • veto on cosmic rays
  • 2 track vertex w/ charge 0
  • reject (coplanar) cosmic rays
  • peak for pt lt 150 MeV/c
  • pp and p-p- give background shape
  • scaled up by 2.1

Signal region ptlt0.15 GeV
  • Preliminary

r0 pt
ptlt0.15 GeV
M(pp-)
20
Minimum Bias Data
200 GeV
  • 800,000 triggers neutron signals in ZDCs
  • Nuclear excitation tags small b interactions
  • excitation and r0 are independent
  • Analysis same as in peripheral

Signal region ptlt0.15 GeV
Preliminary
r0 pt
200 GeV
Preliminary
  • Normalized to 7.2 b hadronic cross section
  • Systematic uncertainties luminosity, overlapping
    events, vertex tracking simulations, single
    neutron selection, etc.

ds/dMpp (mb/GeV)
M(pp-)
21
Summary of Analyses
  • Results
  • Large anisotropic flow, consistent with
    hydrodynamical picture
  • Saturation of v2 at high pt
  • Jet quenching?
  • Suppression of back-to-back jets
  • Surface emission?
  • r0 cross sections measured in ultra-peripheral
    Au-Au collisions, good agreement to theory
  • shown
  • Anisotropic Flow
  • Jets at RHIC
  • Ultra-Peripheral Collisions
  • not shown
  • Particle yields / ratios / spectra
  • Interferometry (HBT)
  • Fluctuations
  • Gluon density saturation
  • Spin physics program

22
RHIC Performance Goals for 2003
  • 29 weeks of d-Au (including cooldown)
  • 8 weeks of p?p?
  • (We wont have Si-Si nor Au-Au next year.)

More interesting physics to come ...
23
STAR Institutions
  • U.S. Labs
  • Argonne, Brookhaven, and Lawrence Berkeley
    National Labs
  • U.S. Universities
  • UC Berkeley, UC Davis, UCLA, Carnegie Mellon,
    Creighton, Indiana, Kent State,
    Michigan State, CCNY, Ohio State, Penn State,
    Purdue, Rice,
  • UT Austin, Texas AM, Valparaiso, Washington,
    Wayne State, Yale
  • Brazil
  • Universidade de Sao Paolo
  • China
  • IPP - Wuhan, IMP - Lanzhou USTC, SINR,
    Tsinghua University, IHEP - Beijing

England University of Birmingham France
IReS - Strasbourg SUBATECH -
Nantes Germany Max Planck Institute - Munich
University of Frankfurt India Institute of
Physics - Bhubaneswar IIT - Mumbai, VECC -
Calcutta Jammu University, Panjab
University University of Rajasthan The
Netherlands NIKHEF Poland Warsaw
University of Technology Russia MEPHI -
Moscow, IHEP - Protvino LPP LHE JINR - Dubna
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