Collision centrality and τ0 dependence of the emission of thermal photons from a fluctuating initial state in an ideal hydrodynamic calculation

Rupa Chatterjee, Hannu Holopainen, Thorsten Renk, and Kari J. Eskola
Phys. Rev. C 85, 064910 – Published 15 June 2012

Abstract

Fluctuations in the initial QCD matter density distribution are found to enhance the production of thermal photons significantly in the range 2pT4 GeV/c compared to a smooth initial state averaged profile in ideal hydrodynamic calculation for 200A GeV Au+Au collisions at the Relativistic Heavy Ion Collider (RHIC) and 2.76A TeV Pb+Pb collisions at the Large Hadron Collider (LHC). The thermal emission of photons is strongly dependent on the initial temperature of the system where the presence of “hot spots” in the initial state translates into enhanced production of photons compared to a smooth profile. The effect of fluctuations in the initial state is found to be stronger for peripheral collisions and for lower beam energies. The pT spectra are found to be quite sensitive to the value of the initial formation time of the plasma which is not known unambiguously and which may vary with collision centralities at a particular beam energy. Increase in the value of the formation time lowers the production of thermal photons compared to the results from a shorter formation time. However, the relative enhancement from fluctuating initial states (compared to a smooth initial state) is found to be stronger for the larger values of formation time. The pT spectra alone are found to be insufficient to quantify the fluctuations in the initial density distribution due to the uncertainties in the initial conditions. A suitably normalized ratio of central-to-peripheral yield as a function of collision centrality and pT can be a useful measure of the fluctuation size scale.

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  • Received 10 April 2012

DOI:https://doi.org/10.1103/PhysRevC.85.064910

©2012 American Physical Society

Authors & Affiliations

Rupa Chatterjee1,*, Hannu Holopainen1,2,3,†, Thorsten Renk1,2,‡, and Kari J. Eskola1,2,§

  • 1Department of Physics, P.O. Box 35, FI-40014 University of Jyväskylä, Finland
  • 2Helsinki Institute of Physics, P.O. Box 64, FI-00014 University of Helsinki, Finland
  • 3Frankfurt Institute for Advanced Studies, Ruth-Moufang-Str. 1, D-60438 Frankfurt am Main, Germany

  • *rupa.r.chatterjee@jyu.fi
  • holopainen@fias.uni-frankfurt.de
  • thorsten.i.renk@jyu.fi
  • §kari.eskola@phys.jyu.fi

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Vol. 85, Iss. 6 — June 2012

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