Toward the determination of heavy-quark transport coefficients in quark-gluon plasma

Shanshan Cao, Gabriele Coci, Santosh Kumar Das, Weiyao Ke, Shuai Y. F. Liu, Salvatore Plumari, Taesoo Song, Yingru Xu, Jörg Aichelin, Steffen Bass, Elena Bratkovskaya, Xin Dong, Pol Bernard Gossiaux, Vincenzo Greco, Min He, Marlene Nahrgang, Ralf Rapp, Francesco Scardina, and Xin-Nian Wang
Phys. Rev. C 99, 054907 – Published 28 May 2019

Abstract

Several transport models have been employed in recent years to analyze heavy-flavor meson spectra in high-energy heavy-ion collisions. Heavy-quark transport coefficients extracted from these models with their default parameters vary, however, by up to a factor of 5 at high momenta. To investigate the origin of this large theoretical uncertainty, a systematic comparison of heavy-quark transport coefficients is carried out between various transport models. Within a common scheme devised for the nuclear modification factor of charm quarks in a brick medium of a quark-gluon plasma, the systematic uncertainty of the extracted drag coefficient among these models is shown to be reduced to a factor of 2, which can be viewed as the smallest intrinsic systematical error band achievable at present time. This indicates the importance of a realistic hydrodynamic evolution constrained by bulk hadron spectra and of heavy-quark hadronization for understanding the final heavy-flavor hadron spectra and extracting heavy-quark drag coefficient. The transverse transport coefficient is less constrained due to the influence of the underlying mechanism for heavy-quark medium interaction. Additional constraints on transport models such as energy loss fluctuation and transverse-momentum broadening can further reduce theoretical uncertainties in the extracted transport coefficients.

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  • Received 24 September 2018

DOI:https://doi.org/10.1103/PhysRevC.99.054907

©2019 American Physical Society

Physics Subject Headings (PhySH)

Particles & FieldsNuclear Physics

Authors & Affiliations

Shanshan Cao1, Gabriele Coci2,3, Santosh Kumar Das4,2, Weiyao Ke5, Shuai Y. F. Liu6, Salvatore Plumari2, Taesoo Song7, Yingru Xu5, Jörg Aichelin8, Steffen Bass5, Elena Bratkovskaya9,10, Xin Dong11, Pol Bernard Gossiaux8, Vincenzo Greco2,3, Min He12, Marlene Nahrgang8, Ralf Rapp6, Francesco Scardina2,3, and Xin-Nian Wang13,11,*

  • 1Department of Physics and Astronomy, Wayne State University, Detroit, Michigan 48201, USA
  • 2Department of Physics and Astronomy, University of Catania, Via Santa Sofia 64, 1-95125 Catania, Italy
  • 3Laboratori Nazionali del Sud, INFN-LNS, Via Santa Sofia 62, I-95123 Catania, Italy
  • 4School of Physical Science, Indian Institute of Technology Goa, Ponda, Goa, India
  • 5Department of Physics, Duke University, Durham, North Carolina 27708, USA
  • 6Cyclotron Institute and Department of Physics and Astronomy, Texas A&M University, College Station, Texas 77843, USA
  • 7Institut für Theoretische Physik, Universität Gießen, Germany
  • 8SUBATECH, IMT Atlantique, Université de Nantes, CNRS-IN2P3, Nantes, France
  • 9Institute for Theoretical Physics, Johann Wolfgang Goethe Universität, Frankfurt am Main, Germany
  • 10GSI Helmholtzzentrum für Schwerionenforschung GmbH, Darmstadt, Germany
  • 11Nuclear Science Division, Lawrence Berkeley National Laboratory, Berkeley, California 94740, USA
  • 12Department of Applied Physics, Nanjing University of Science and Technology, Nanjing 210094, China
  • 13Key Laboratory of Quark and Lepton Physics (MOE) and Institute of Particle Physics, Central China Normal University, Wuhan 430079, China

  • *xnwang@lbl.gov

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Vol. 99, Iss. 5 — May 2019

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