Cosmological Scenarios with Bounce and Genesis in Horndeski Theory and Beyond

被引:14
|
作者
Volkova, V. E. [1 ]
Mironov, S. A. [1 ,2 ,3 ]
Rubakov, V. A. [1 ,4 ]
机构
[1] Russian Acad Sci, Inst Nucl Res, Moscow 117312, Russia
[2] Moscow MV Lomonosov State Univ, Inst Theoret & Math Phys, Moscow 119991, Russia
[3] Alikhanov Inst Theoret & Expt Phys, Moscow 117218, Russia
[4] Moscow MV Lomonosov State Univ, Phys Fac, Moscow 119991, Russia
基金
俄罗斯科学基金会;
关键词
Cosmology;
D O I
10.1134/S1063776119100236
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
This essay is a brief review of the recent studies of non-singular cosmological scenarios with bounce and Genesis and their stability in a subclass of scalar-tensor theories with higher derivatives-beyond Horndeski theories. We discuss the general results of stability analysis of the nonsingular cosmological solutions in beyond Horndeski theories, as well as other closely related topics: 1) the no-go theorem, which is valid in the general Horndeski theories but not in their extensions, 2) singularities in disformal transformations relating beyond Horndeski theories with general ones, 3) healthy behavior of the scalar sector in the unitary gauge despite divergencies of coefficients in the quadratic action for perturbations ("gamma-crossing"). We describe several specific examples of bouncing cosmologies and models with Genesis epoch which have neither ghosts nor gradient instabilities among the linearized perturbations about the homogeneous isotropic background during entire evolution.
引用
收藏
页码:553 / 565
页数:13
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