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Slajd 1

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???????????? ?????????? ? ??????????? p0-??????? ? ??????? ???????????? ... BRAHMS & PP2PP. STAR. PHENIX. AGS. LINAC. BOOSTER. Pol. H- Source. Spin Rotators ... – PowerPoint PPT presentation

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Title: Slajd 1


1
???????????? ?????????? ? ??????????? p0-???????
? ??????? ???????????? ??????????????? ??????????
????? ?? ????????? ???? ? ???????????
?.?????, ????, ????????the STAR Collaboration
2
Motivation
  • Contrary to simple pQCD predictions, first
    measurements of ? production in p?p collisions
    found large transverse single-spin asymmetries.
    Similar large effects have recently been found in
    ee- and semi-inclusive deep-inelastic
    scattering.
  • Significant developments in theory in the past
    few years suggest common origins for these
    effects, but large transverse spin asymmetries in
    p?p ? ? X production are not yet fully
    understood.

3
Possible mechanisms
  • Sivers effect Phys. Rev. D 41, 83 (1990) 43,
    261 (1991)
  • Flavor dependent correlation between the
    proton spin (Sp), proton momentum (Pp) and
    transverse momentum (kT) of the unpolarized
    partons inside. The unpolarized parton
    distribution function fq(x,kT) is modified to
  • Collins effect Nucl. Phys. B396, 161 (1993)
  • Correlation between the quark spin (sq),
    quark momentum (pq) and transverse momentum (kT)
    of the pion. The fragmentation function of
    transversely polarized quark q takes the form

According to the latest theoretical developments,
both mechanisms contribute to ?? AN
4
RHIC Polarized Collider
RHIC pC Polarimeters
Absolute Polarimeter (H? jet)
BRAHMS PP2PP
PHOBOS
Siberian Snakes
Siberian Snakes
PHENIX
STAR
Spin Rotators (longitudinal polarization)
Spin Rotators (longitudinal polarization)
Pol. H- Source
LINAC
BOOSTER
Helical Partial Siberian Snake
AGS
200 MeV Polarimeter
AGS pC Polarimeter
Strong AGS Snake
1 MHz collision rate Polarization 0.5-0.6
5
STAR detector layout
Forward Meson Spectrometer
  • TPC -1.0 lt ? lt 1.0
  • FTPC 2.8 lt ??? lt 3.8
  • BBC 2.2 lt ??? lt 5.0
  • EEMC 1 lt ? lt 2
  • BEMC -1 lt ? lt 1

FPD/FPD ? -3.7/3.3
FPD/FMS ? -4.1/2.5-4.0
1/2 of the FMS
6
Transverse spin runs at STAR with forward
calorimetry 2001?2008
sampled
7
Single Spin Asymmetry
  • Definition
  • ds?(?) differential cross section of p0
    when incoming proton has spin up(down)
  • Two methods of measurements
  • Single arm calorimeter
  • R relative luminosity (by BBC)
  • Pbeam beam polarization
  • Two arm (left-right) calorimeter
  • No relative luminosity needed

positive AN more p0 going left to polarized beam
8
Detectors from FPD to FMS
  • Run8 and beyond FMS
  • FMS provides full azimuthal coverage for range
    2.5 ? h ? 4.0
  • broad acceptance in xF-pT plane for inclusive
    g,p0,w,K0, production in pp and d(p)Au
  • broad acceptance for g-p0 and p0-p0 from
    forward jet pairs
  • Runs 3-6 FPD, FPD
  • Inclusive p0 cross sections
  • AN for inclusive p0 production

three different positions of modular detectors
20x more acceptance then previous detectors
single monolithic detector
9
Published measurements with FPD
PRL 92, 171801 (2004)
  • PRL 101, 222001 (2008)
  • Large transverse single-spin asymmetries at large
    xF
  • xF dependence matches Sivers effect expectations
    qualitatively
  • pT dependence at fixed xF is not consistent with
    1/pT expectation of theoretical model calculations

vs200 GeV, lt?gt 3.8
Asymmetry revealed at lower energies persists at
vs200 GeV
10
Run8 data analysis -calibration
  • the calibration methodologies employed for the
    FPD have been successfully adapted to the FMS
  • offline cell-by-cell calibration using p0 peak
    position in the sorted by high tower mass
    distributions
  • Event selection done with

minbias condition hightower ADC
threshold (400/200 cts. for small/large cells)
(for small cells only) fiducial volume cut (0.5
cell)
11
LED monitoring system
Minimal time dependence in p0 peak position is
observed
LED system critical calibration tool
Calorimeter stable at the level of a few
percents
12
Data to simulations comparison
  • Full PYTHIA/GEANT simulations have adequate
    statistics to reach moderate xF
  • Mass resolution in data is reasonable, given
    Run6 FPD performance
  • Simulations have somewhat better resolution
    than data

DATA
SIMULATION
Present understanding sufficient further
investigations to be done
13
First look at p0 AN from Run8 data
STAR preliminary
stat.errors only
75 of Run8 data
Octant subdivision of FMS for inclusive p0 spin
sorting
  • AN comparable to prior measurements
  • Azimuthal variation appears to be as expected

14
Summary
  • High precision AN measurements with the FPD
    allows for a quantitative comparison with
    theoretical models.
  • FMS was commissioned and fully operated in Run8.
    It has 20x the acceptance of FPD (1264 channels
    compared to 98 for the pair of FPD modules).
  • Reconstruction and calibration procedures
    successfully ported from FPD to FMS.
  • Calibration is completed and data show good
    agreement with the simulated sample of events.
  • Inclusive p0 AN(xF) from the FMS is in agreement
    with the FPD measurements.

15
Outlook
  • Complete analysis of p0 asymmetry
  • Going beyond p0 detection
  • - AN for a state that contains p0 pairs
  • - AN for states with heavier mesons
  • (?, ?, J/?)
  • - direct photons, jet-like events can
    help
  • to discriminate between Sivers and
  • Collins effects

16
BACKUP
17
p0 cross section measurements
PRL 97, 152302 (2006)
Cross-section is consistent with NLO pQCD
calculations it was used in a recent global
analysis of ee-, SIDIS and pp data to determine
fragmentation functions PR D76, 074033 (2007)
18
Separating Sivers and Collins effects
Collins mechanism asymmetry in the forward jet
fragmentation
Sivers mechanism asymmetry in the forward jet or
? production
SP
SP
kT,q
p
p
p
p
Sq
kT,p
Sensitive to proton spin parton transverse
motion correlations
Sensitive to transversity
To discriminate between the two effects we need
to go beyond p0 detection to direct photons or
jet-like events
19
Energy dependent corrections
  • p0 peak position depends on the energy
  • linear correction extracted from p0 peak
    position and being applied to photon energies
    works for both p0s and ?s, and significantly
    decreases shift from zero in dE?? Esimu -
    Ereco.

20
Association analysis
  • comparison of generated quantities to GEANT
    simulations
  • we consider

CORRECTED
UNCORRECTED
Eliminating energy dependence in p0 mass peak
gives the correct average neutral pion energy
21
Simulation and search algorithm for p0p0 in FMS
and its engineering prototype
  • it is possible to find events where the p0 pair
    originated at a significant distance from the
    vertex
  • one source of such events are decays KS?p0p0
    (31 branching fraction)
  • plot shows the mass distribution for displaced
    vertices above 100 cm from the BBC vertex a
    pronounced KS mass bump is visible
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