Classical gluon radiation in ultrarelativistic nuclear collisions: Space-time structure, instabilities, and thermalization

Sergei G. Matinyan, Berndt Müller, and Dirk H. Rischke
Phys. Rev. C 57, 1927 – Published 1 April 1998
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Abstract

We investigate the space-time structure of the classical gluon field produced in an ultrarelativistic collision between color charges. The classical solution which was computed previously in a perturbative approach is shown to become unstable on account of the non-Abelian self-interaction neglected in the perturbative solution scheme. The time scale for growth of the instabilities is found to be of the order of the distance between the colliding color charges. We argue that these instabilities will eventually lead to thermalization of gluons produced in an ultrarelativistic collision between heavy nuclei. The rate of thermalization is estimated to be of order g2μ, where g is the strong coupling constant and μ2 the transverse color charge density of an ultrarelativistic nucleus.

  • Received 28 August 1997

DOI:https://doi.org/10.1103/PhysRevC.57.1927

©1998 American Physical Society

Authors & Affiliations

Sergei G. Matinyan1,2, Berndt Müller1, and Dirk H. Rischke1

  • 1Department of Physics, Duke University, Box 90305, Durham, North Carolina 27708-0305
  • 2Yerevan Physics Institute, Yerevan 375036, Armenia

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Vol. 57, Iss. 4 — April 1998

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