Measurement of Open Charm Mesons in 200 GeV Heavy Ion Collisions at STAR
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Measurement of Open Charm Mesons in 200 GeV Heavy Ion Collisions at STAR. Stephen Baumgart Yale University. Outline. Charm Cross-Section in Cu+Cu Motivation Analysis Procedure Results D s Measurement Detector Charge Asymmetry Question. Theory Motivation.

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Measurement of Open Charm Mesons in 200 GeV Heavy Ion Collisions at STAR

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Measurement of open charm mesons in 200 gev heavy ion collisions at star

Measurement of Open Charm Mesons in 200 GeV Heavy Ion Collisions at STAR

Stephen Baumgart

Yale University


Outline

Outline

  • Charm Cross-Section in Cu+Cu

    • Motivation

    • Analysis Procedure

    • Results

  • Ds Measurement

    • Detector

    • Charge Asymmetry Question


Theory motivation

Theory Motivation

  • Prediction of Charm Cross Section in p+p from QCD (NLO/FONLL)

    • Deviations from prediction in Cu+Cu, Au+Au collisions will show medium effects.

      Ref: M. Cacciari, P. Nason, R. Vogt, Phys. Rev. Lett. 95, 122001 (2005)

  • Charm production is a good probe of early state of medium

    • Charm produced during initial gluon fusion

    • Charm produced before thermalization.

      Ref: Kuznetsova, J. Rafelski Eur. Phys. J. C 51, 113-133(2007)

Basic Gluon Fusion Diagram


Theoretical uncertainties

Theoretical Uncertainties

  • Prediction 1

  • use dpt slices, then integrate final result

  • treat charm as active flavor

Charm Cross Section Predicted for 200 GeV Collisions:

  • Prediction 2

  • calculate on full pt range in one step

  • treat charm as NOT an active flavor (heavy quark considered massive)

Charm Cross Section Predicted for 200 GeV Collisions:

  • Ref: R. Vogt, arXiv:0709.2531v1 [hep-ph]

The large error bars mean that experimental measurements are needed

to help constrain theoretical predictions.

Our STAR measurements will help resolve these discrepancies.


D 0 to k p analysis method in cu cu minbias collisions

D0 to Kp Analysis Method in Cu+Cu MinBias Collisions

Kaon Tracks

Pion Tracks

Unused Tracks

D0 Mass

Combinatorial Technique

Rotational Background Subtraction

or Event Mixing Background Subtraction

py

p

Momentum and dE/dx cuts used

px

K

5 degree

rotations

13 rotations


D 0 d 0 in minimum bias cu cu

D0 + D0 in Minimum Bias Cu+Cu

STAR Preliminary

For Kp pairs:

|y| < 1.0

pt < 4.0 GeV/c


D 0 d 0 2 spectra in minimum bias cu cu

( D0 + D0)/2Spectra in Minimum Bias Cu+Cu

|y| < 1.0

77% of area under curve is between 0.3 and 3.3 GeV/c!

Fitting Function:

*Systematic error evaluation for dN/dy in progress.


Conversion from dn dy to cross section

Conversion from dN/dy to Cross-Section

number of binary collisions

p+p inelastic cross section

conversion to full rapidity

(using PYTHIA simulation, ver. 6.152)

ratio from e+e- collider data

*Systematic error evaluation for dN/dy in progress.


Charm cross section comparison at 200 gev

Charm Cross-Section Comparison at 200 GeV

  • NLO Ref: R. Vogt, arXiv:0709.2531v1 [hep-ph]

STAR:

C. Adler, et al. Phys. Rev. Lett. 91 172302 (2003)

S. Baumgart, arXiv:nucl-ex/0709.4223

Y. Zhang, arXiv:nucl-ex/0607011

*Systematic error evaluation for STAR Cu+Cu in progress.

PHENIX:

S. Adler, et al. Phys. Rev. Lett. 94 082301 (2005)

S. Adler, et al. Phys. Rev. Lett. 97 252002 (2005)


D s motivation

Ds Motivation

D/Ds ratio predicted by stat. hadronization model.

Can be tested in STAR.


Svt secondary vertexing

SVT Secondary Vertexing

  • Use SVT to find secondary vertices of Ds to fpdecay (ct = 149.9 mm).

  • Use mass cut on f to eliminate background.


The d s charge asymmetry

The Ds Charge Asymmetry

d+Au Ds+

Cu+Cu Ds+

d+Au Ds-

Cu+Cu Ds-


Conclusions

Conclusions

  • The charm cross-section measured in Cu+Cu is consistent with other STAR charm cross-section measurements assuming binary scaling.

  • Current evidence suggests there may be many more Ds+ than Ds- ; however, more statistics are urgently needed.

  • New Au+Au and d+Au dataset are coming up!


D 0 reconstruction in simulation backup

D0 Reconstruction in Simulation (Backup)

The D0 peak can be successfully recreated in simulation.


D 0 from kp in d au au au backup

D0 from Kp in d+Au & Au+Au (Backup)

D0 measured via Kp channel in Au+Au, d+Au.

pt spectra obtained, yields measured.

Counts

D0 Peak Reconstructed from Kp in Au+Au,

STAR Preliminary

D0 Peak Reconstructed from Kp in d+Au,

STAR Collaboration, J. Adams et al., Phys. Rev. Lett. 94, 062301 (2005).


Comparison to phenix electrons backup

Comparison to PHENIX Electrons (Backup)

PHENIX and STAR: RAA for Non-photonic e±

central Au+Au, √sNN=200 GeV

Electron RAA matches PHENIX but not Yields!

Red Circles and

Blue Triangles = STAR

Open Circles = PHENIX

PHENIX: PRL 98 (2007) 172301

STAR: PRL 98 (2007) 192301

DVGL: Djordjevic, Phys. Lett. B 632 (2006) 81

BDMPS: Armesto, Phys. Lett. B 637 (2006) 362

Phys. Rev. Lett. 98, 192301 (2007)


Results from non photonic electrons backup

Results from Non-Photonic Electrons (Backup)

  • The pt spectrum of open charm to electrons has been measured out to high pt.

  • Non-photonic electron measurements allow open charm spectra to be extended to high pt.

B. I. Abelev et al, Phys. Rev. Lett. 98 (2007) 192301


Open charm via semi leptonic decays backup

Open Charm via Semi-Leptonic Decays (Backup)

  • Simulations show that high pt non-photonic electrons come almost exclusively from charm decays.

  • We use the STAR Electromagnetic Calorimeter (EMCAL) to detect these electrons.

  • Electrons from photonic conversions are cut from the sample.

  • Method is insensitve to details of the intervening material between interaction region and detector.

black: e+e- pairs

blue: comb. background

red=photonic e±=black – blue

Invariant Mass [GeV/c2]


Measuring open charm via muons backup

Measuring Open Charm via Muons (Backup)

  • Muons are detected by the STAR Time-of-Flight (TOF) detector.

  • The muon measurement constrains the open charm yield at low pt.

Muon Points

Y. Zhang, arXiv:nucl-ex/0607011

Procedure Reference: H.D. Liu et. al., Phys. Lett.B 639, 441 (2006)


Heavy ion collisions backup

Heavy Ion Collisions (Backup)

  • Collisions in p+p, d+Au, Cu+Cu, Au+Au

  • Beam Energies of sq. root(SNN) = 20, 62, 130, 200 GeV

  • High Multiplicities relative to particle physics experiments


Star detector at rhic backup

STAR Detector at RHIC (Backup)

The Relativistic Heavy Ion Collider

The Relativistic Heavy Ion Collider (RHIC) is located at Brookhaven, New York.

RHIC uses p+p, d+A, and A+A beams.

The STAR Detector

1)

The Solenoidal Tracker at RHIC (STAR) is one of four major detectors.

Beam Line

  • Three Ways to Study Open Charm:

  • Direct Hadronic Measurement (TPC)

  • Electron Measurement (EMCAL)

  • Muon Measurement (TOF)

2)

3)


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