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.


 

HF Meeting 2016/12/15 - update for QM17

 

Status of D* measurement in p+p run 15

Status of D* measurement in p+p run 15

Baldin ISHEPP XXIII Proceeding

Baldin ISHEPP XXIII Proceeding

sPHENIX performance study based on Fast Simulation

 

HIJING production for Run14 NPE analysis

Production reqeusts

1. 1M Events for test production with MB (0-15fm), |Vz| < 6cm 
2. Output file : PicoDst
3.

Poster abstract for QM2017 v2

 Poster abstract for QM2017 v2

Hard Probe 2016

 

Preliminary plots for J/psi analysis in pp 500GeV

 

Poster abstract for QM2017

 Poster abstract for QM2017 - D0 meson in Cu+Au

Poster abstract for QM2017

 Poster abstract for QM2017 - D0 meson in Cu+Au

Abstract for IBSHEPP 2016

Abstract for IBSHEPP 2016.

BCmeeting presentation

 

Run15 QA check

 

Abstract for Hard Probes 2016

 

HF PWG meeting 20160623

HF PWG meeting 20160602

IWND2016

 

PicoDst QA Run16065027 (test)

 

HF PWG meeting 20160331

 

Presentation on D-h work