BARYOGENESIS IN EXTENDED INFLATION .2. BARYOGENESIS VIA PRIMORDIAL BLACK-HOLES

被引:109
作者
BARROW, JD
COPELAND, EJ
KOLB, EW
LIDDLE, AR
机构
[1] NASA,FERMILAB ASTROPHYS CTR,FERMI NATL ACCELERATOR LAB,BATAVIA,IL 60637
[2] UNIV CHICAGO,ENRICO FERMI INST,DEPT ASTRON & ASTROPHYS,CHICAGO,IL 60637
来源
PHYSICAL REVIEW D | 1991年 / 43卷 / 04期
关键词
D O I
10.1103/PhysRevD.43.984
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
This is the second of two papers devoted to the study of baryogenesis at the end of extended inflation. Extended inflation is brought to an end by the collisions of bubble walls surrounding regions of true vacuum, a process which produces particles well out of thermal equilibrium. In the first paper we considered baryogenesis via direct production and subsequent decay of baryon-number-violating bosons. In this paper we consider the further possibility that the wall collisions may provide a significant density of primordial black holes and examine their possible role in generating a baryon asymmetry.
引用
收藏
页码:984 / 994
页数:11
相关论文
共 33 条
[31]   MATTER-ANTIMATTER ACCOUNTING, THERMODYNAMICS, AND BLACK-HOLE RADIATION [J].
TOUSSAINT, D ;
TREIMAN, SB ;
WILCZEK, F ;
ZEE, A .
PHYSICAL REVIEW D, 1979, 19 (04) :1036-1045
[32]   BARYON PRODUCTION BY PRIMORDIAL BLACK-HOLES [J].
TURNER, MS .
PHYSICS LETTERS B, 1979, 89 (01) :155-159
[33]   SOME PROBLEMS WITH EXTENDED INFLATION [J].
WEINBERG, EJ .
PHYSICAL REVIEW D, 1989, 40 (12) :3950-3959