Warm baryogenesis

被引:53
作者
Bastero-Gil, Mar [2 ]
Berera, Arjun [1 ]
Ramos, Rudnei O. [3 ]
Rosa, Joao G. [1 ]
机构
[1] Univ Edinburgh, SUPA, Sch Phys & Astron, Edinburgh EH9 3JZ, Midlothian, Scotland
[2] Univ Granada, Dept Fis Teor & Cosmos, E-18071 Granada, Spain
[3] Univ Estado Rio de Janeiro, Dept Fis Teor, BR-20550013 Rio De Janeiro, RJ, Brazil
关键词
Baryogenesis; Dissipation; Warm inflation; Grand Unified theories; INFLATIONARY UNIVERSE; COSMOLOGY; SCENARIO; FLATNESS; HORIZON; MODEL;
D O I
10.1016/j.physletb.2012.05.032
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We show that a baryon asymmetry can be generated by dissipative effects during warm inflation via a supersymmetric two-stage mechanism, where the inflaton is coupled to heavy mediator fields that then decay into light species through B- and CP-violating interactions. In contrast with thermal GUT baryogenesis models, the temperature during inflation is always below the heavy mass threshold, simultaneously suppressing thermal and quantum corrections to the inflaton potential and the production of dangerous GUT relics. This naturally gives a small baryon asymmetry close to the observed value, although parametrically larger values may be diluted after inflation along with any gravitino overabundance. Furthermore, this process yields baryon isocurvature perturbations within the range of future experiments, making this an attractive and testable model of GUT baryogenesis. (C) 2012 Elsevier B.V. All rights reserved.
引用
收藏
页码:425 / 429
页数:5
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