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Pibero Djawotho

Publications and source records attributed to Pibero Djawotho.

3 recordsLinked to original sources

Gluon polarization and jet production at STAR

At RHIC kinematics, polarized jet hadroproduction is dominated by $gg$ and $qg$ scattering, making the jet longitudinal double-spin asymmetry, $A_{LL}$, sensitive to gluon polarization in the nucleon. I will present STAR results of $A_{LL}$ from inclusive jet and dijet measurements for the RHIC 2006 run totaling 5.5 pb$^{-1}$ of integrated luminosity with 55% beam polarization at center-of-mass energy 200 GeV. I will also present preliminary results from the analyses of data from the 2009 run, which collected a much larger sample (25 pb$^{-1}$ with 57% polarization) at 200 GeV. The results are compared with theoretical calculations of $A_{LL}$ based on various models of the polarized gluon distribution function in the nucleon. The STAR data place significant constraints on allowed theoretical models.

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Gluon polarization measurements with inclusive jets at STAR

At RHIC kinematics, polarized jet hadroproduction is dominated by $gg$ and $qg$ scattering, making the jet double longitudinal spin asymmetry, $A_{LL}$, sensitive to gluon polarization in the nucleon. I will present STAR results of $A_{LL}$ from inclusive jet measurements for the RHIC 2006 run at center-of-mass energy 200 GeV. I will also discuss the current status of the analysis of data from the 2009 run, also at center-of-mass energy 200 GeV. The results are compared with theoretical calculations of $A_{LL}$ based on various models of the gluon density in the nucleon. The STAR data place significant constraints on allowed theoretical models.

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Upsilon cross section in p+p collisions at STAR

The main focus of the heavy flavor program at RHIC is to investigate the properties of the dense matter produced in heavy-ion collisions by studying its effect on open heavy flavor and quarkonia production. This in turn requires a detailed understanding of their production in elementary p+p collisions so that the dense matter effects can be later unfolded. In this paper, we present the first mid-rapidity cross section measurement of bottomonium at $\sqrt{s}=200$ GeV with the STAR experiment. We compare our results with perturbative QCD calculations. A brief status on the study of charmonium in STAR is given.

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