Gravitational baryogenesis

被引：193

作者：

Davoudiasl, H ^{[1
]}

Kitano, R ^{[1
]}

Kribs, GD ^{[1
]}

Murayama, H ^{[1
]}

Steinhardt, PJ ^{[1
]}

机构：

[1] Inst Adv Study, Sch Nat Sci, Princeton, NJ 08540 USA

来源：

PHYSICAL REVIEW LETTERS | 2004年 / 93卷 / 20期

基金：

美国国家科学基金会;

关键词：

D O I：

10.1103/PhysRevLett.93.201301

中图分类号：

O4 [物理学];

学科分类号：

0702 ;

摘要：

We show that a gravitational interaction between the derivative of the Ricci scalar curvature and the baryon-number current dynamically breaks CPT in an expanding Universe and, combined with baryon-number-violating interactions, can drive the Universe towards an equilibrium baryon asymmetry that is observationally acceptable.

引用

页码：201301 / 1

页数：4

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