Post inflation reheating in an expanding universe
Jul, 199517 pages
Published in:
- Phys.Rev.D 53 (1996) 1776-1783
- Published: 1996
e-Print:
- astro-ph/9507108 [astro-ph]
Report number:
- HUTP-95-A027,
- DART-HEP-95-04
View in:
Citations per year
Abstract: (arXiv)
An analytic means of studying the resonant decay of the inflaton field is developed for the case of background expansion, H=0. It is shown that the parametric resonance in the inflaton's decay need not disappear when the expansion of the universe is taken into account, although the total number of particles produced is fewer than in the H≃0 case.- inflation
- chaos
- postulated particle: inflaton
- decay: inflaton
- inflaton: decay
- resonance
- expansion: background
- field theory: scalar
- particle: production
- production: particle
References(35)
Figures(0)
- •
- Phys.Rev.D 23 (1981) 347-356,
- Adv.Ser.Astrophys.Cosmol. 3 (1987) 139-148 (reprint)
- •
- Phys.Rev.Lett. 48 (1982) 1220-1223,
- Adv.Ser.Astrophys.Cosmol. 3 (1987) 158-161 (reprint)
- •
- Phys.Lett.B 108 (1982) 389-393,
- In *Moscow 1981, Proceedings, Quantum Gravity*, 185-195 and Moscow Inst. Phys. Acad. Sci. - 81-229 (81,REC.DEC.) 15p,
- Adv.Ser.Astrophys.Cosmol. 3 (1987) 149-153 (reprint)
- •
- Phys.Lett.B 117 (1982) 29,
- In *Abbott, L.F. (ed.), Pi, S.Y. (ed.): Inflationary cosmology*, 436-440. (Phys. Lett. B117 (1982) 29-33) and MIT Cambridge - CTP-0983 (82,rec.Jul.) 18 p
- ,
- ,
- ,
- •
- Phys.Rev.Lett. 48 (1982) 1437,
- In *Abbott, L.F. (ed.), Pi, S.Y. (ed.): Inflationary cosmology*, 441-444. (Phys. Rev. Lett. 48 (1982) 1437-1440). (see Book Index)
- •
- Phys.Lett.B 116 (1982) 329,
- In *Abbott, L.F. (ed.), Pi, S.Y. (ed.): Inflationary cosmology*, 430-435. (Phys. Lett. B116 (1982) 329-334) and Moscow Inst. Theor. Exp. Phys. GKAE - ITEF-82-078 (82,rec.Jul.) 16 p. (207206) (see Book Index)
- •
- Phys.Lett.B 129 (1983) 177-181,
- Reprinted in *Abbott, L.F. (ed.), Pi, S.Y. (ed.): Inflationary cosmology*, 37-41
- •
- Phys.Rev.D 42 (1990) 2491-2504
- Sov.J.Nucl.Phys. 51 (1990) 172-177,
- Yad.Fiz. 51 (1990) 273-282,
- Yad. Fiz. 51 (1990) 273-282 and Dubna JINR - 89-321 (89,rec.Jul.) 14 p
- ,
- ,
- •
- Phys.Rev.Lett. 73 (1994) 3195-3198
- e-Print:•
- •
- Phys.Rev.D 51 (1995) 2693-2702
- e-Print:•
- •
- Prog.Theor.Phys. 94 (1995) 873-898
- e-Print:•
- DOI:
- JETP Lett. 41 (1985) 493-496,
- Pisma Zh.Eksp.Teor.Fiz. 41 (1985) 402-405,
- Pisma Zh. Eksp. Teor. Fiz. 41 ( 1985) 402-405
- •
- Phys.Lett.B 218 (1989) 17-20
- ,
- ,
- •
- Phys.Rept. 215 (1992) 203-333
- •
- Prog.Theor.Phys. 76 (1986) 1036
- DOI:
- •
- Phys.Rev.D 48 (1993) 3544-3556
- •
- Astrophys.J. 427 (1994) 542-561
- DOI:
- •
- Phys.Rept. 231 (1993) 1-105
- e-Print:•
- •
- Proc.Roy.Soc.Lond.A 360 (1978) 117-134
- •
- J.Phys.A 11 (1978) 1315-1328
- •
- Nucl.Phys.B 245 (1984) 328,
- Nucl. Phys. B245 ( 1984) 328-342 and Calif. Univ. Santa Barbara - NSF-ITP-84-003 (84,REC.FEB.) 24 P. (403312)
- •
- Phys.Rev.D 32 (1985) 1899-1920,