Preequilibrium evolution of a non-Abelian plasma

Physical Review D - Particles, Fields, Gravitation and Cosmology

Volumn 55, Issue 11, 1997, Pages 6877-6886

  Nayak, Gouranga C ^a   Ravishankar, V ^a  

^a INDIAN INSTITUTE OF TECHNOLOGY   (India)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 0000473266     PISSN: 15507998     EISSN: 15502368     Source Type: Journal    
DOI: 10.1103/PhysRevD.55.6877     Document Type: Article

References (31)

1. J. Stachel and G. R. Young, Annu. Rev. Nucl. Part. Sci. 42, 537 (1992).
2. J. Schukraft, Nucl. Phys. A583, 673c (1995).
3. M. Jacob, Int. J. Mod. Phys. A 6, 2569 (1991), and references therein.
4. R. C. Hwa and M. T. Nazirov, Phys. Rev. Lett. 69, 741 (1992);
5. A. K. Mohanty and S. Kataria, 73, 2672 (1994).
6. T. Matsui and H. Satz, Phys. Lett. B 178, 416 (1986).
7. J. Rafelski and B. Muller, Phys. Rev. Lett. 48, 1066 (1982);
8. C. P. Singh, 56, 870 (1990).
9. M. T. Strickland, Phys. Lett. B 331, 245 (1994).
10. M. Jacob, Nucl. Phys. A583, 13c (1995).
11. G. Baym, Phys. Lett. 138B, 18 (1984).
12. J. D. Bjorken, Phys. Rev. D 27, 140 (1983).
13. See, e.g., R. V. Gavai, in Proceedings of the DAE Symposium on High Energy Physics, Bombay, India, 1992, edited by S. Banerjee and P. Roy (Indian Academy of Science, Bombay, 1993).
14. K. Kajantie and T. Matsui, Phys. Lett. 164B, 373 (1985).
15. J. Schwinger, Phys. Rev. 82, 664 (1951).
16. A. Bialas et al., Nucl. Phys. B296, 611 (1988).
17. B. Banerjee, R. S. Bhalerao, and V. Ravishankar, Phys. Lett. B 224, 16 (1989).
18. M. Asakawa and T. Matsui, Phys. Rev. D 43, 2871 (1991).
19. K. Geiger and J. Kapusta, Phys. Rev. D 47, 4905 (1993).
20. U. Heinz, Phys. Rev. Lett. 51, 351 (1983).
21. T. T. Wu and C. N. Yang, Phys. Rev. D 12, 3843 (1975).
22. R. V. Gavai (private communication).
23. F. E. Low, Phys. Rev. D 12, 163 (1975).
24. S. Nussinov, Phys. Rev. Lett. 34, 1286 (1975).
25. S. K. Wong, Nuovo Cimento A 65, 689 (1970).
26. R. Pisarski, Phys. Rev. Lett. 63, 1129 (1989).
27. P. F. Kelly, Q. Liu, C. Lucchesi, and C. Manuel, Phys. Rev. Lett. 72, 3461 (1994).
28. P. F. Kelly, Q. Liu, C. Lucchesi, and C. Manuel, Phys. Rev. D 50, 4209 (1994).
29. A perturbative source term which would arise for time-dependent fields will not alter the situation since it is of order (Formula presented).
30. (Formula presented) can also be made weakly local. See H. Heiselberg and X. N. Wang, Phys. Rev. C 53, 1892 (1996).
31. B. Svetitsky, Phys. Rev. D 37, 2484 (1988).