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Cosmological viable models in f(T,B) gravity as solutions to the H₀ tension

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arxiv 1909.10328 v2 pith:2NR6PKCO submitted 2019-09-20 gr-qc astro-ph.COhep-thphysics.data-an

Cosmological viable models in $f(T,B)$ gravity as solutions to the $H_0$ tension

Celia Escamilla-Rivera , Jackson Levi Said This is my paper
classification gr-qc astro-ph.COhep-thphysics.data-an
keywords cosmologicalgravitylatemodelstheoryviableaccelerationaccording
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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abstract

In this work we present a further investigation about Teleparallel Gravity Cosmology. We demonstrate that according the current astrophysical data (CC+Pantheon+BAO samplers with late universe measurements SH0ES+H0LiCOW), an $f(T,B)$ theory can provide another interpretation to the oscillatory behaviour of the dark energy equation of state when applied to late times. The four $f(T,B)$ 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 $\Lambda$CDM model.

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Cited by 3 Pith papers

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