Abstract. In this article we report on the results of quarkonia production in p+p, d+Au, and Au+Au collisions at midrapidity via the dielectron decay channel at √ s N N = 200 GeV from STAR. Results from J/ψ production in p+p collisions for pT < 14 GeV/c are presented to provide a baseline for studying suppression in heavy ion collisions and are also used to understand the quarkonium production mechanism. The nuclear modification factor for J/ψ in d+Au collisions for pT < 5 GeV/c and Au+Au collisions for pT < 10 GeV/c is reported, along with J/ψ elliptic flow v2 in Au+Au collisions. The results from Υ(1S+2S+3S) production in p+p and Au+Au collisions are also provided, and the Upsilon nuclear modification factor in Au+Au collisions is presented.
IntroductionThe production of heavy quarkonia has been extensively used to probe the hot and dense medium created in heavy ion collisions, as they are expected to be suppressed in a deconfined medium due to the Debye screening of the heavy quark potential [1]. Because of their large mass, heavy quarks are primarily created in the initial hard scattering of the collision and provide information about the early stages and the evolution of the system. There are however various modifications other than color-screening to quarkonium production in heavy ion collisions, such as the recombination of charm quarks [2] into bound-state charmonium, formation time effects where high transverse momentum (p T ) particles may escape from the suppression region [3], and modifications to feeddown and sequential melting of excited states [4] There are further modifications to quarkonium production in heavy ion collisions from Cold Nuclear Matter effects (CNM) [5], such as modifications to parton distribution functions (PDFs) inside the nucleus (shadowing) [6], and nuclear absorption [7]. To disentangle all of these effects, a quantitative understanding of J/ψ and Υ production in p + A, d + A, and A+A is required. In this article, the results for J/ψ production in p+p, d+Au, and Au+Au collisions at √ s N N = 200 GeV from the STAR detector are reported. The J/ψ p T spectrum and nuclear