Thermal leptogenesis and gauge mediation

被引:32
作者
Fujii, M [1 ]
Ibe, M
Yanagida, T
机构
[1] Univ Tokyo, Dept Phys, Tokyo 1130033, Japan
[2] Univ Tokyo, Res Ctr Early Universe, Tokyo 1130033, Japan
来源
PHYSICAL REVIEW D | 2004年 / 69卷 / 01期
关键词
D O I
10.1103/PhysRevD.69.015006
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We show that a minithermal inflation occurs naturally in a class of gauge mediation models of supersymmetry (SUSY) breaking, provided that the reheating temperature T-R of the primary inflation is much higher than the SUSY-breaking scale, say T-R>10(10) GeV. The reheating process of the thermal inflation produces an amount of entropy, which dilutes the number density of relic gravitinos. This dilution renders the gravitino to be the dark matter in the present Universe. The abundance of the gravitinos is independent of the reheating temperature T-R, once the gravitinos are thermally produced after the reheating of the primary inflation. We find that the thermal leptogenesis takes place at T(L)similar or equal to10(12)-10(14) GeV for m(3/2)similar or equal to100 keV-10 MeV without any gravitino problem.
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页数:9
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