Restriction to parametric resonant decay after inflation

被引:25
作者
Kasuya, S
Kawasaki, M
机构
[1] Institute for Cosmic Ray Research, University of Tokyo, Tanashi
关键词
induced decay; parametric resonance; reheating;
D O I
10.1016/S0370-2693(96)01216-6
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We study parametric resonant decay of inflaton field with emphasis on its physical meaning. We show that the parametric resonance is indeed an induced process, which means that the more numbers of produced particles, the more inflaton field decays. We also consider the dissipative effects of produced particles and find that the dissipation reduces the resonant decay rate of inflaton field.
引用
收藏
页码:686 / 691
页数:6
相关论文
共 21 条
[1]   PARTICLE-PRODUCTION IN THE NEW INFLATIONARY COSMOLOGY [J].
ABBOTT, LF ;
FARHI, E ;
WISE, MB .
PHYSICS LETTERS B, 1982, 117 (1-2) :29-33
[2]   COSMOLOGY FOR GRAND UNIFIED THEORIES WITH RADIATIVELY INDUCED SYMMETRY-BREAKING [J].
ALBRECHT, A ;
STEINHARDT, PJ .
PHYSICAL REVIEW LETTERS, 1982, 48 (17) :1220-1223
[3]   DISSIPATION VIA PARTICLE-PRODUCTION IN SCALAR FIELD-THEORIES [J].
BOYANOVSKY, D ;
DEVEGA, HJ ;
HOLMAN, R ;
LEE, DS ;
SINGH, A .
PHYSICAL REVIEW D, 1995, 51 (08) :4419-4444
[4]   Linear versus nonlinear relaxation: Consequences for reheating and thermalization [J].
Boyanovsky, D ;
DAttanasio, M ;
deVega, HJ ;
Holman, R ;
Lee, DS .
PHYSICAL REVIEW D, 1995, 52 (12) :6805-6827
[5]  
BOYANOVSKY D, 1995, PITT0995
[6]  
BOYANOVSKY D, 1995, IN PRESS P SCH STRIN
[7]   BARYON ASYMMETRY IN THE INFLATIONARY UNIVERSE [J].
DOLGOV, AD ;
LINDE, AD .
PHYSICS LETTERS B, 1982, 116 (05) :329-334
[8]  
DOLGOV AD, 1990, SOV J NUCL PHYS+, V51, P172
[9]  
FUJISAKI H, 1995, TU95493
[10]  
FUJISAKI H, 1995, TU95488