Export citation

Export citation

Choose format for download:

Download Citation
  • Access by Xinjiang University

Non-Abelian plasma instabilities for extreme anisotropy

Peter Arnold

Guy D. Moore

  • Department of Physics, University of Virginia, P.O. Box 400714, Charlottesville, Virginia 22904-4714, USA

  • Department of Physics, McGill University, 3600 rue University, Montréal, Québec H3A 2T8, Canada

Phys. Rev. D 76, 045009 – Published 17 August, 2007

DOI: https://doi.org/10.1103/PhysRevD.76.045009

Abstract

Thermalization of quark-gluon plasmas in heavy-ion collisions is a difficult theoretical problem. One theoretical goal has been to understand the physics of thermalization in the relatively simplifying limit of arbitrarily high energy collisions, where the running coupling αs is weak. One of the current roadblocks to achieving this goal is lack of knowledge about the behavior of plasma instabilities when particle distributions are highly anisotropic. In particular, it has not been known how the magnetic fields generated by plasma instabilities scale with anisotropy. In this paper, we use numerical simulations in a first attempt to determine this scaling.

Article Text

References (25)

  1. R. Baier, A. H. Mueller, D. Schiff, and D. T. Son, Phys. Lett. B 502, 51 (2001).
  2. P. Arnold, J. Lenaghan, and G. D. Moore, J. High Energy Phys. 08 (2003) 002.
  3. S. Mrówczyński, Phys. Lett. B 214, 587 (1988); Y. E. Pokrovsky and A. V. Selikhov, Pis’ma Zh. Eksp. Teor. Fiz. 47, 11 (1988) [JETP Lett. 47, 12 (1988)]; Yad. Fiz. 52, 229 (1990) [Sov. J. Nucl. Phys. 52, 146 (1990)]; Yad. Fiz. 52, 605 (1990) [Sov. J. Nucl. Phys. 52, 385 (1990)]; O. P. Pavlenko, Yad. Fiz. 55, 2239 (1992) [Sov. J. Nucl. Phys. 55, 1243 (1992)]; S. Mrówczyński, Phys. Lett. B 314, 118 (1993); Phys. Rev. C 49, 2191 (1994); Phys. Lett. B 393, 26 (1997).
  4. P. Romatschke and M. Strickland, Phys. Rev. D 68, 036004 (2003).
  5. E. S. Weibel, Phys. Rev. Lett. 2, 83 (1959).
  6. A. Rebhan, P. Romatschke, and M. Strickland, Phys. Rev. Lett. 94, 102303 (2005).
  7. A. Rebhan, P. Romatschke, and M. Strickland, J. High Energy Phys. 09 (2005) 041.
  8. P. Romatschke and R. Venugopalan, Phys. Rev. Lett. 96, 062302 (2006); Phys. Rev. D 74, 045011 (2006).
  9. A. Dumitru and Y. Nara, Phys. Lett. B 621, 89 (2005).
  10. A. Dumitru, Y. Nara, and M. Strickland, Phys. Rev. D 75, 025016 (2007).
  11. D. Bödeker and K. Rummukainen, arXiv:0705.0180.
  12. P. Arnold, G. D. Moore, and L. G. Yaffe, Phys. Rev. D 72, 054003 (2005).
  13. P. Arnold and G. D. Moore, Phys. Rev. D 73, 025006 (2006).
  14. D. Bödeker, J. High Energy Phys. 10 (2005) 092.
  15. P. Arnold and G. D. Moore, Phys. Rev. D 73, 025013 (2006).
  16. S. Mrówczyński and M. H. Thoma, Phys. Rev. D 62, 036011 (2000).
  17. P. Arnold, G. D. Moore, and L. G. Yaffe, J. High Energy Phys. 01 (2003) 030.
  18. A. H. Mueller, A. I. Shoshi, and S. M. H. Wong, Nucl. Phys. B760, 145 (2007).
  19. P. Romatschke and A. Rebhan, Phys. Rev. Lett. 97, 252301 (2006).
  20. S. Mrówczyński, A. Rebhan, and M. Strickland, Phys. Rev. D 70, 025004 (2004).
  21. D. Bödeker, G. D. Moore, and K. Rummukainen, Phys. Rev. D 61, 056003 (2000).
  22. P. Arnold and J. Lenaghan, Phys. Rev. D 70, 114007 (2004).
  23. Berndt Müller (private communication).
  24. N. K. Nielsen and P. Olesen, Nucl. Phys. B144, 376 (1978).
  25. P. Arnold and P. S. Leang, arXiv:0704.3996 [Phys. Rev. D (to be published)].

Sign In to Your Journals Account

Filter

Filter

Article Lookup

Enter a citation