The Polonyi problem and upper bound on inflation scale in supergravity

被引:39
作者
Ibe, M.
Shinbara, Y. [1 ]
Yanagida, T. T.
机构
[1] Univ Tokyo, Dept Phys, Tokyo 1130033, Japan
[2] Univ Tokyo, Res Ctr Early Universe, Tokyo 1130033, Japan
基金
日本学术振兴会;
关键词
D O I
10.1016/j.physletb.2006.06.041
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We reconsider the Polonyi problem in gravity-mediation models for supersymmetry (SUSY) breaking. It has been argued that there is no problem in the dynamical SUSY breaking scenarios, since the Polonyi field acquires a sufficiently large mass of the order of the dynamical SUSY-breaking scale Lambda(SUSY). However, we find that a linear term of the Polonyi field in the Kahler potential brings us back to the Polonyi problem, unless the inflation scale is sufficiently low, H-inf less than or similar to 10(8) GeV, or the reheating temperature is extremely low, T-R less than or similar to 100 GeV. Here, this Polonyi problem is more serious than the original one, since the Polonyi field mainly decays into a pair of gravitinos. (c) 2006 Elsevier B.V. All rights reserved.
引用
收藏
页码:534 / 540
页数:7
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