Cosmological viable models inf(T,B)theory as solutions to theH0tension

被引：72
作者：
Escamilla-Rivera, Celia [1 ]
Said, Jackson Levi [2 ,3 ]
机构：
[1] Univ Nacl Autonoma Mexico, Inst Ciencias Nucl, AP 70-543, Mexico City 04510, DF, Mexico
[2] Univ Malta, Inst Space Sci & Astron, MSD-2080 Msida, Malta
[3] Univ Malta, Dept Phys, MSD-2080 Msida, Malta
来源：
CLASSICAL AND QUANTUM GRAVITY | 2020年 / 37卷 / 16期
基金：
欧盟地平线“2020”;
关键词：
cosmology; H(0)tension; modified gravity; BARYON ACOUSTIC-OSCILLATIONS; GRAVITATIONAL ENERGY; DARK ENERGY; RECONSTRUCTION; GALAXIES; DISTANCE; GRAVITY; TORSION;
D O I：
10.1088/1361-6382/ab939c
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
In this work we present a further investigation about teleparallel gravity cosmology. We demonstrate that according to the current astrophysical data (CC + Pantheon + BAO samplers with late Universe measurements SH0ES + H0LiCOW), anf(T,B) theory can provide another interpretation to the oscillatory behaviour of the dark energy equation of state when applied to late times. The fourf(T,B) cosmological viable models proposed here can undergo an epoch of late-time acceleration and reproduce quintessence and phantom regimes with a transition along the phantom-divided line, making this theory a good approach to modify the standard ?CDM model.
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页数：28
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