Superheavy dark matter in R2-cosmology

被引:2
|
作者
Arbuzova, E., V [1 ,2 ]
机构
[1] Dubna State Univ, Dept Higher Math, Univ Skaya Str 19, Dubna 141983, Russia
[2] Novosibirsk State Univ, Dept Phys, Pirogova Str 2, Novosibirsk 630090, Russia
来源
基金
俄罗斯科学基金会;
关键词
Dark matter; inflation; scalaron; RADIOACTIVE DECAY;
D O I
10.1142/S0218271821400022
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The conventional Friedmann cosmology is known to be in tension with the existence of stable particles having interaction strength typical for supersymmetry and heavier than several TeV. A possible way to save life of such particles may be a modification of the standard cosmological expansion law in such a way that the density of these heavy relics would be significantly reduced. We study particle creation in the Starobinsky inflationary model for different decay channels of the scalaron. It is shown that the process of thermalization superheavy stable particles with the coupling strength typical for the GUT SUSY could be created with the density equal to the observed density of dark matter.
引用
收藏
页数:9
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