Out of equilibrium dynamics of an inflationary phase transition

Physical Review D - Particles, Fields, Gravitation and Cosmology

Volumn 55, Issue 6, 1997, Pages 3373-3388

  Boyanovsky, D ^a   Cormier, D ^b   de Vega, H J ^c   Holman, R ^b  

^a UNIVERSITY OF PITTSBURGH   (United States)

^b CARNEGIE MELLON UNIVERSITY   (United States)

^c LPTHE   (France)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 0000218556     PISSN: 15507998     EISSN: 15502368     Source Type: Journal    
DOI: 10.1103/PhysRevD.55.3373     Document Type: Article

References (52)

1. A. H. Guth, Phys. Rev. D23, 347 (1981).
2. A. H. Guth and E. J. Weinberg, Nucl. Phys.B212, 321 (1983);
3. S. W. Hawking, I. Moss, and J. Stewart, Phys. Rev. D26, 2681 (1982).
4. A. D. Linde, Phys. Lett.108B, 389 (1982).
5. A. Albrecht and P. J. Steinhardt, Phys. Rev. Lett.48, 1220 (1982).
6. A. D. Linde, Phys. Lett.129B, 177 (1983).
7. For reviews of inflationary cosmology, see R. H. Brandenberger, Rev. Mod. Phys.57, 1 (1985);
8. Int. J. Mod. Phys. A2, 77 (1987).
9. L. Abbott and S-Y. Pi, Inflationary Cosmology (World Scientific, Singapore, 1986).
10. E. W. Kolb and M. S. Turner, The Early Universe (Addison Wesley, Redwood City, CA, 1990).
11. A. Linde, Particle Physics and Inflationary Cosmology (Harwood Academic Publishers, Chur, Switzerland, 1990). For a recent summary of inflationary cosmology, see A. Linde, in Current Topics in Astrofundamental Physics, Proceedings of the Chalonge Erice School, edited by N. Sánchez and A. Zichichi, NATO ASI series C Vol. 467 (Kluwer Academic, Dordrecht, 1995);A. Linde, in Particles, Strings and Cosmology: proceedings, edited by J. Bagger (World Scientific, Singapore, 1996).
12. For reviews on topological defects in early universe cosmology, see A. Vilenkin and E. P. S. Shellard, Cosmic Strings and Other Topological Defects (Cambridge University Press, Cambridge, England, 1994);
13. M. B. Hindmarsh and T. W. B. Kibble, Rep. Prog. Phys.58, 477 (1995).
14. A. Vilenkin, Phys. Lett.115B, 91 (1982).
15. A. D. Linde, Phys. Lett.116B, 335 (1982).
16. A. Vilenkin and L. H. Ford, Phys. Rev. D26, 1231 (1982).
17. A. Vilenkin, Nucl. Phys.B226, 504 (1983);
18. B226, 527 (1986).
19. G. F Mazenko, W. G. Unruh, and R. M. Wald, Phys. Rev. D31, 273 (1985);
20. G. F. Mazenko, Phys. Rev. Lett.54, 2163 (1985).
21. A. Guth and S.-Y. Pi, Phys. Rev. D32, 1899 (1985).
22. For a thorough exposition of nonequilibrium methods in cosmology see, for example, E. Calzetta and B. L. Hu, Phys. Rev. D35, 495 (1987);
23. 37, 2838 (1988);
24. J. P. Paz, 41, 1054 (1990);
25. 42, 529 (1990);B. L. Hu, in Bauff/Cap Workshop on Thermal Field Theories: proceedings, edited by F. C. Khanna, R. Kobes, G. Kunstatter, and H. Umezawa (World Scientific, Singapore, 1994), p. 309; and in the Proceedings of the Second Paris Cosmology Colloquium, Observatoire de Paris, 1994, edited by H. J. de Vega and N. Sánchez (World Scientific, Singapore, 1995), p. 111, and references therein.
26. A. Ringwald, Ann. Phys. (N.Y.)177, 129 (1987); APNYA6
27. Phys. Rev. D36, 2598 (1987).
28. H. Leutwyler and S. Mallik, Ann. Phys. (N.Y.)205, 1 (1991).APNYA6
29. G. Semenoff and N. Weiss, Phys. Rev. D31, 699 (1985).
30. For nonequilibrium methods in different contexts see, for example, F. Cooper, J. M. Eisenberg, Y. Kluger, E. Mottola, and B. Svetitsky, Phys. Rev. Lett.67, 2427 (1991);
31. Phys. Rev. D48, 190 (1993).
32. F. Cooper and E. Mottola, Mod. Phys. Lett. A2, 635 (1987);
33. F. Cooper, S. Habib, Y. Kluger, E. Mottola, J. P. Paz, and P. R. Anderson, Phys. Rev. D50, 2848 (1994);
34. F. Cooper, S.-Y. Pi, and P. N. Stancioff, 34, 3831 (1986);
35. F. Cooper, Y. Kluger, E. Mottola, and J. P. Paz, 51, 2377 (1995);
36. F. Cooper and E. Mottola, 36, 3114 (1987).
37. O. Eboli, R. Jackiw, and S-Y. Pi, Phys. Rev. D37, 3557 (1988);
38. M. Samiullah, O. Eboli, and S-Y. Pi, 44, 2335 (1991).
39. J. Guven, B. Liebermann, and C. Hill, Phys. Rev. D39, 438 (1989).
40. D. Boyanovsky, H. J. de Vega, and R. Holman, Phys. Rev. D49, 2769 (1994).
41. D. Boyanovsky, H. J. de Vega, R. Holman, D.-S. Lee, and A. Singh, Phys. Rev. D51, 4419 (1995);
42. D. Boyanovsky, M. D’Attanasio, H. J. de Vega, R. Holman, and D. S. Lee, 52, 6805 (1995);
43. D. Boyanovsky, M. D’Attanasio, H. J. de Vega, and R. Holman, 54, 1748 (1996);
44. D. Boyanovsky, H. J. de Vega, R. Holman, and J. Salgado, 54, 7570 (1996);D. Boyanovsky, D. Cormier, H. J. de Vega, R. Holman, A. Singh, and M. Srednicki, “Preheating in FRW Universes,” Report No. hep-ph/9609527, 1996 (unpublished).For reviews see D. Boyanovsky, H. J. de Vega, and R. Holman, in Proceedings of the Second Paris Cosmology Colloquium, Observatoire de Paris, 1994, edited by H. J. de Vega and N. Sánchez (World Scientific, Singapore, 1995), pp. 127–215;D. Boyanovsky, M. D’Attanasio, H. J. de Vega, R. Holman, and D.-S. Lee, in Proceedings of the Erice Chalonge School, “String Gravity and Physics at the Planck Energy Scale,” NATO Advanced Study Institute, edited by N. Sánchez and A. Zichichi (Kluwer, Dordrecht, 1996), pp. 451–492.
45. D. Boyanovsky and H. J. de Vega, Phys. Rev. D47, 2343 (1993).
46. D. Boyanovsky, D-S. Lee, and A. Singh, Phys. Rev. D48, 800 (1993).
47. F. Cooper, S. Habib, Y. Kluger, and E. Mottola, Phys. Rev. D (to be published).
48. F. Cooper and E. Mottola, Mod. Phys. Lett. A2, 635 (1987).
49. T. S. Bunch and P. C. W. Davies, Proc. R. Soc. London, INSA360, 117 (1978); see also Ref. 32.
50. N. D. Birrell and P. C. W. Davies, Quantum Fields in Curved Space (Cambridge University Press, Cambridge, England, 1986).
51. P. R. Anderson, Phys. Rev. D32, 1302 (1985.)
52. See, for example, the recent review by J. E. Lidsey, A. R. Liddle, E. W. Kolb, E. J. Copeland, T. Barreiro, and M. Abney, “Reconstructing the Inflaton Potential—an overview,” Report No. Fermilab Pub 95-280-A, astro-ph/9508078, 1995 (unpublished).