Preheating in quintessential inflation

被引：34

作者：

Campos, AH ^{[1
]}

Reis, HC

Rosenfeld, R

机构：

[1] Univ Sao Paulo, Inst Fis, Dept Fis Nucl, BR-66318 Sao Paulo, SP, Brazil

[2] Univ Estadual Campinas, Inst Fis Gleb Wataghin, Dept Raios Cosmicos & Cronol, BR-6165 Campinas, SP, Brazil

[3] Univ Nacl Estadual Sao Paulo, Inst Fis Teor, BR-01405900 Sao Paulo, Brazil

来源：

PHYSICS LETTERS B | 2003年 / 575卷 / 3-4期

基金：

巴西圣保罗研究基金会;

关键词：

D O I：

10.1016/j.physletb.2003.09.064

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We perform a numerical study of the preheating mechanism of particle production in models of quintessential inflation and compare it with the usual gravitational production mechanism. We find that even for a very small coupling between the inflaton field and a massless scalar field, g greater than or similar to 10(-6), preheating dominates over gravitational particle production. Reheating temperatures in the range 10(4) less than or similar to T-rh less than or similar to 10(15) GeV can be easily obtained. (C) 2003 Published by Elsevier B.V.

引用

页码：151 / 156

页数：6

共 14 条

[1]

[Anonymous], JHEP

[2]

DIAS AG, HEPPH0204121

[3] Modeling quintessential inflation [J].

Dimopoulos, K ;

Valle, JWF .

ASTROPARTICLE PHYSICS, 2002, 18 (03) :287-306

[4]

DOLGOV AD, 1990, SOV J NUCL PHYS+, V51, P172

[5]

FARRAR GR, ASTROPH307316

[6] Instant preheating [J].

Felder, G ;

Kofman, L ;

Linde, A .

PHYSICAL REVIEW D, 1999, 59 (12)

[7] Inflation and preheating in nonoscillatory models [J].

Felder, G ;

Kofman, L ;

Linde, A .

PHYSICAL REVIEW D, 1999, 60 (10)

[8] GRAVITATIONAL PARTICLE CREATION AND INFLATION [J].

FORD, LH .

PHYSICAL REVIEW D, 1987, 35 (10) :2955-2960

[9] Towards the theory of reheating after inflation [J].

Kofman, L ;

Linde, A ;

Starobinsky, AA .

PHYSICAL REVIEW D, 1997, 56 (06) :3258-3295

[10]

Linde A.D., 1990, PARTICLE PHYS INFLAT, V5, P1

← 1 2 →