Generic Modification of Gravity, Late Time Acceleration and Hubble Tension

被引:17
作者
Gangopadhyay, Mayukh R. [1 ]
Pacif, Shibesh K. Jas [1 ]
Sami, Mohammad [1 ,2 ,3 ]
Sharma, Mohit K. [1 ]
机构
[1] SGT Univ, Ctr Cosmol & Sci Popularizat CCSP, Gurugram 122505, India
[2] Eurasian Natl Univ, Ctr Theoret Phys, Astana 010008, Kazakhstan
[3] Chinese Acad Sci, 52 Sanlihe Rd, Beijing 100045, Peoples R China
关键词
modified gravity; hubble tension; dark Energy; phantom crossing; DARK ENERGY; COSMOLOGICAL CONSTANT; H-0; CONSTRAINTS; SUPERNOVAE; PARAMETER; DYNAMICS; UNIVERSE; LAMBDA; MODELS;
D O I
10.3390/universe9020083
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We consider a scenario of large-scale modification of gravity that does not invoke extra degrees of freedom, but includes coupling between baryonic matter and dark matter in the Einstein frame. The total matter energy density follows the standard conservation, and evolution has the character of deceleration in this frame. The model exhibits interesting features in the Jordan frame realised by virtue of a disformal transformation where individual matter components adhere to standard conservation but gravity is modified. A generic parametrization of disformal transformation leaves thermal history intact and gives rise to late time acceleration in the Jordan frame, which necessarily includes phantom crossing, which, in the standard framework, can be realised using at least two scalar fields. This scenario is embodied by two distinguished features, namely, acceleration in the Jordan frame and deceleration in the Einstein frame, and the possibility of resolution of the Hubble tension thanks to the emergence of the phantom phase at late times.
引用
收藏
页数:20
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