Heavy Flavor

Depending on the energy scale, there are two mechanisms that generate quark masses with different degrees of importance: current quark masses are generated by the electroweak symmetry breaking mechanism (Higgs mass) and spontaneous chiral symmetry breaking leads to the constituent quark masses in QCD (QCD mass). The QCD interaction strongly affects the light quarks (u, d, s) while the heavy quark masses (c, b, t) are mainly determined by the Higgs mechanism. In high-energy nuclear collisions at RHIC, heavy quarks are produced through gluon fusion and qq¯ annihilation. Heavy quark production is also sensitive to the parton distribution function. Unlike the light quarks, heavy quark masses are not modified by the surrounding QCD medium (or the excitations of the QCD medium) and the value of their masses is much higher than the initial excitation of the system. It is these differences between light and heavy quarks in a medium that make heavy quarks an ideal probe to study the properties of the hot and dense medium created in high-energy nuclear collisions.

 

Heavy flavor analyses at STAR can be separated into quarkonia, open heavy flavor and heavy flavor leptons.


 

PXL calibration

Speaker : Michael Lomnitz


Talk time : 13:30, Duration : 00:20

 

Upsilon pp, dAu, AuAu GPC E-mail Responses

 This is a page to house long e-mail responses.

Presentations

 Page for uploading presentation drafts.

STAR Regional Meeting: Heavy Quark Production and Correlations 2012

2012-11-04
2012-11-06
Poland
-
from Monday, 5 November 2012 to Wednesday, 7 November 2012
Faculty of Physics, Warsaw University of Technology, Warsaw
Conference organizing committee information :
  • Jaroslav Bielcik (CTU)
  • Martin Girard (WUT)
  • Adam Kisiel (WUT)
  • Leszek Kosarzewski (WUT)
  • Grazyna Odyniec (LBNL)
  • Piotr Ostrowski (WUT)
  • Tomasz Pawlak (WUT)
  • Jan Pluta (WUT)
  • Michal Sumbera (NPI)
  • Barbara Trzeciak (WUT)
  • Hanna Zbroszczyk (WUT) - Chairperson
Conference duration: 3 days

STAR Regional Meeting: Heavy Quark Production and Correlations 2012 takes place at Faculty of Physics of Warsaw University of Technology

Upsilon pp, dAu, AuAu Paper Documents

 This page is for collecting the following documents related to the Upsilon pp (2009), dAu (2008) and AuAu (2010) paper:

Upsilon Paper: pp, d+Au, Au+Au

 Page to collect the information for the Upsilon paper based on the analysis of

Upsilon Analysis in p+p 2009 - L0 Trigger

D0/D* 500 GeV p+p

Speaker : David Tlusty


Talk time : 11:30, Duration : 00:30

J/Psi polarization (EVO)

Upsilon Analysis in d+Au 2008

Upsilon yield and nuclear modification factor in d+Au collisions at sqrt(s)=200 GeV.

PAs: Anthony Kesich, and Manuel Calderon de la Barca Sanchez.

 

Upsilon Analysis in p+p 2009

Upsilon cross-section in p+p collisions at sqrt(sNN) = 200 GeV, 2009 data.

Update on J/psi polarization study

Speaker : Barbara Trzeciak ( WUT )


Talk time : 14:00, Duration : 00:45

Response to PRD referee comments on Upsilon Paper

First Round of Referee Responses

Click here for second round.

e-h correlation in Run9 500 GeV

Speaker : Wei Li ( SINAP/UCLA )


Talk time : 16:15, Duration : 00:30

Embedding Discussion

NPE analysis in run 2008 d+Au

Speaker : Wenqin Xu ( UCLA )


Talk time : 16:15, Duration : 00:30

Varying the Continuum Contribution to the Dielectron Mass Spectrum

Initial Normalization

Estimating Drell-Yan contribution from NLO calculation.

Ramona calculated the cross section for DY at NLO and sent the data points to us.  These were first shown in the RHIC II Science Workshop, April 2005, in her Quarkonium

Code to run Pythia and produce b-bbar -> e+ e- events

// main00.cc
// Modified from the main01.cc
// which is a part of the PYTHIA event generator.
// Copyright (C) 2008 Torbjorn Sjostrand.

Using Pythia 8 to get b-bbar -> e+e-

We used Pythia 8 to produce b-bbar events. First we used the default Pythia 8.