Nonperturbative quantum dynamics of a new inflation model

Physical Review D - Particles, Fields, Gravitation and Cosmology

Volumn 57, Issue 4, 1998, Pages 2166-2185

  Boyanovsky, D ^a   Cormier, D ^a   de Vega, H J ^a   Holman, R ^a   Kumar, S P ^a  

^a UNIVERSITY OF PITTSBURGH   (United States)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 0000918667     PISSN: 15507998     EISSN: 15502368     Source Type: Journal    
DOI: 10.1103/PhysRevD.57.2166     Document Type: Article

References (62)

1. A. H. Guth, Phys. Rev. D 23, 347 (1981).
2. N. Turok, Ue-Li Pen, and U. Seljak, “The Scalar, Vector and Tensor Contributions to CMB anisotropies from Topological Defects,” astro-ph/9706250, 1997.
3. Andreas Albrecht, Richard A. Battye, and James Robinson, Phys. Rev. Lett. 79, 4736 (1997).
4. B. Allen, R. R. Caldwell, S. Dodelson, L. Knox, E. P. S. Shellard, and A. Stebbins, Phys. Rev. Lett. 79, 2624 (1997).
5. For thorough reviews of standard and inflationary cosmology see E. W. Kolb and M. S. Turner, The Early Universe (Addison Wesley, Redwood City, CA, 1990).
6. A. Linde, Particle Physics and Inflationary Cosmology (Harwood Academic, Chur, Switzerland, 1990).
7. R. Brandenberger, Rev. Mod. Phys. 57, 1 (1985).
8. R. BrandenbergerInt. J. Mod. Phys. A 2, 77 (1987).
9. For more recent reviews see M. S. Turner, astro-ph/9703197.
10. M. S. Turnerastro-ph/9703196.
11. M. S. Turnerastro-ph/9703174.
12. M. S. Turnerastro-ph/9703161.
13. M. S. Turnerastro-ph/9704062.
14. M. S. Turnerastro-ph/9704024.
15. A. Linde, in Current Topics in Astrofundamental Physics, Proceedings of the Chalonge Erice School, edited by N. Sánchez and A. Zichichi (NATO Advanced Study Institute, Series C, Vol. 467), Dordrecht, 1995)(Kluwer Academic.
16. A. R. Liddle, astro-ph/9612093, presented at the Casablanca Winter School.
17. A. R. Liddle and D. H. Lyth, Phys. Rep. 231, 1 (1993).
18. G. Smoot, astro-ph/9705135.
19. M. Sakellariadou, astro-ph/9612075, and references therein.
20. D. H. Lyth, hep-ph/9609431, 1996.
21. S. Dodelson, W. H. Kinney, and E. W. Kolb, Phys. Rev. D 56, 3207 (1997).
22. D. Boyanovsky, H. J. de Vega, R. Holman, D.-S. Lee, and A. Singh, Phys. Rev. D 51, 4419 (1995).
23. Phys. Rev. DD. Boyanovsky, H. J. de Vega, R. Holman, and J. F. J. Salgado, 54, 7570 (1996).
24. D. Boyanovsky, H. J. de Vega, and R. Holman, in Proceedings of the Erice Chalonge School on Astrofundamental Physics, edited by N. Sánchez and A. Zichichi (World Scientific, Singapore, 1997) pp. 183–270.
25. D. Boyanovsky, H. J. de Vega, and R. Holman, Phys. Rev. D 49, 2769 (1994).
26. D. Boyanovsky, D. Cormier, H. J. de Vega, and R. Holman, Phys. Rev. D 55, 3373 (1997).
27. D. Boyanovsky, D.-S. Lee, and A. Singh, Phys. Rev. D 48, 800 (1993).
28. D. Boyanovsky, D. Cormier, H. J. de Vega, R. Holman, A. Singh, and M. Srednicki, Phys. Rev. D 56, 1939 (1997).
29. A. D. Linde, Phys. Lett. 116B, 335 (1982).
30. A. Vilenkin, Phys. Lett. 115B, 91 (1982).
31. P. J. Steinhardt and M. S. Turner, Phys. Rev. D 29, 2162 (1984).
32. A. Guth and S-Y. Pi, Phys. Rev. D 32, 1899 (1985).
33. N. D. Birrell and P. C. W. Davies, Quantum Fields in Curved Space (Cambridge University Press, Cambridge, England, 1986).
34. O. Eboli, R. Jackiw, and S-Y. Pi, Phys. Rev. D 37, 3557 (1988).
35. Phys. Rev. DM. Samiullah, O. Eboli, and S-Y. Pi, 44, 2335 (1991).
36. J. Guven, B. Liebermann, and C. Hill, Phys. Rev. D 39, 438 (1989).
37. 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).
38. F. CooperJ. M. EisenbergY. KlugerE. MottolaB. SvetitskyPhys. Rev. D 48, 190 (1993).
39. F. Cooper and E. Mottola, Mod. Phys. Lett. A 2, 635 (1987).
40. F. Cooper, S. Habib, Y. Kluger, E. Mottola, J. P. Paz, and P. R. Anderson, Phys. Rev. D 50, 2848 (1994).
41. Phys. Rev. DF. Cooper, S.-Y. Pi, and P. N. Stancioff, 34, 3831 (1986).
42. Phys. Rev. DF. Cooper, Y. Kluger, E. Mottola, and J. P. Paz, 51, 2377 (1995).
43. Phys. Rev. DF. Cooper and E. Mottola, 36, 3114 (1987).
44. S. A. Ramsey and B. L. Hu, Phys. Rev. D 56, 678 (1997).
45. J. Baacke, K. Heitmann, and C. Patzold, Phys. Rev. D 56, 6556 (1997).
46. Phys. Rev. DJ. BaackeK. HeitmannC. Patzold55, 2320 (1997).
47. D. Polarski and A. A. Starobinsky, Class. Quantum Grav. 13, 377 (1996).
48. J. Lesgourgues, D. Polarski, and A. A. Starobinsky, Nucl. Phys. B497, 479 (1997), and references therein.
49. L. P. Grishchuk, Phys. Rev. D 45, 4717 (1992).
50. V. F. Mukhanov, H. A. Feldman, and R. H. Brandenberger, Phys. Rep. 215, 293 (1992).
51. J. Bardeen, Phys. Rev. D 22, 1882 (1980).
52. R. R. Caldwell, Class. Quantum Grav. 13, 2437 (1995).
53. J. Martin and D. J. Schwarz, gr-qc/9704049, 1997.
54. K. M. Gorski, A. J. Banday, C. L. Bennett, G. Hinshaw, A. Kogut, and G. F. Smoot, astro-ph/9601063.
55. L. P. Grishchuk, Phys. Rev. D 52, 5549 (1995); in Proceedings of the NATO Advanced Study Institute on “String Gravity and Physics at the Planck Scale,” edited by N. Sanchez and A. Zichichi (NATO Advanced Study Institute, Series C, Vol. 476) (Kluwer, Dordrecht, 1996), p. 369.
56. Phys. Rev. D 53, 6784 (1996);in Proceedings of the NATO Advanced Study Institute on “Current Topics in Astrofundamental Physics: the Early Universe,” edited by N. Sanchez and A. Zichichi (NATO Advanced Study Institute, Series C, Vol. 467) (Kluwer, Dordrecht, 1995), p. 205.
57. J. E. Lidsey, A. R. Liddle, E. W. Kolb, E. J. Copeland, T. Barreiro, and M. Abney, Rev. Mod. Phys. 69, 373 (1997).
58. E. D. Stewart and D. H. Lyth, Phys. Lett. B 302, 171 (1993).
59. S. Habib, Phys. Rev. D 46, 2408 (1992).
60. Phys. Rev. DS. Habib42, 2566 (1990).
61. Phys. Rev. DS. Habib and R. Laflamme, 42, 4056 (1990), and references therein.
62. See Eq. (53) in the first reference in 28.