Magneto-sonoluminescence and its signatures in photon and dilepton production in relativistic heavy ion collisions

Gökçe Başar, Dmitri E. Kharzeev, and Edward V. Shuryak
Phys. Rev. C 90, 014905 – Published 14 July 2014

Abstract

The matter produced in the early stages of heavy ion collisions consists mostly of gluons, and is penetrated by the coherent magnetic field produced by spectator nucleons. The fluctuations of gluonic matter in an external magnetic field couple to real and virtual photons through virtual quark loops. We study the resulting contributions to photon and dilepton production that stem from the fluctuations of the stress tensor Tμν in the background of a coherent magnetic field B. Our study extends significantly the earlier work [G. Basar, D. E. Kharzeev, and V. Skokov, Phys. Rev. Lett. 109, 202303 (2012)], in which only the fluctuations of the trace of the stress tensor Tμμ were considered (the coupling of Tμμ to electromagnetic fields is governed by the scale anomaly). In the present paper we derive more general relations using the operator product expansion (OPE). We also extend the previous study to the case of dileptons, which offers the possibility to discriminate between various production mechanisms. Among the phenomena that we study are magneto-sonoluminescence [MSL, the interaction of magnetic field B(x,t) with the sound perturbations of the stress tensor δTμν(x,t)] and magneto-thermoluminescence [MTL, the interaction of B(x,t) with smooth average Tμν]. We calculate the rates of these process and find that they can dominate the photon and dilepton production at early stages of heavy ion collisions. We also point out the characteristic signatures of MSL and MTL that can be used to establish their presence and to diagnose the produced matter.

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  • Received 21 March 2014
  • Revised 24 May 2014

DOI:https://doi.org/10.1103/PhysRevC.90.014905

©2014 American Physical Society

Authors & Affiliations

Gökçe Başar1, Dmitri E. Kharzeev1,2, and Edward V. Shuryak1

  • 1Department of Physics and Astronomy, Stony Brook University, Stony Brook, New York 11794, USA
  • 2Department of Physics, Brookhaven National Laboratory, Upton, New York 11973, USA

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Vol. 90, Iss. 1 — July 2014

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