Matter and antimatter asymmetry in a rainbow universe

被引:2
|
作者
Atazadeh, K. [1 ]
机构
[1] Azarbaijan Shahid Madani Univ, Dept Phys, Tabriz 53714161, Iran
关键词
Rainbow gravity; Gravitational baryogenesis; BLACK-HOLE; HAWKING RADIATION; GRAVITY; BARYOGENESIS; THERMODYNAMICS; RELATIVITY;
D O I
10.1016/j.aop.2022.169133
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
In rainbow gravity, the ordinary general relativity (GR) field equations can be modified by a parametric set of equations and thus the cosmology of this scenario may give new sounds about the physics of the early universe. As we know in the radiation -dominated universe the gravitational baryogenesis mechanism (GBM) cannot occur in the GR context. In this regard, by as-suming the flat Friedmann-Robertson-Walker (FRW) metric we study GBM in the rainbow gravity. We obtain that for a rainbow universe filled with radiation, the baryon-to-entropy ratio from the GBM can have a non-zero value. In this work, we study the baryon-to-entropy ratio for the corresponding cosmological models of two suggested dispersion relations and we obtain that in the first case the baryogenesis mechanism occurs and also the results are compatible with the observational constraints while the second case is not consistent with the observational constraints.(c) 2022 Elsevier Inc. All rights reserved.
引用
收藏
页数:9
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