Inflation and the B-L breaking scale

被引：0

作者：

Jeannerot, R ^{[1
]}

机构：

[1] Univ Sussex, Ctr Theoret Phys, Brighton BN1 9QH, E Sussex, England

来源：

COSMO-97: FIRST INTERNATIONAL WORKSHOP ON PARTICLE PHYSICS AND THE EARLY UNIVERSE | 1998年

关键词：

D O I：

暂无

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Inflation arises in supersymmetric grand unified theories (susy GUTs) without fine tuning and cosmic strings usually form at the end of inflation. Hence both strings and inflation contribute to the density perturbations in the very early universe which lead to structure formation and to CMB anisotropies. This may give us a hint as to the B - L breaking scale.

引用

页码：380 / 382

页数：3

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