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

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

Celia Escamilla-Rivera , Jackson Levi Said This is my paper · ORCID
classification gr-qcastro-ph.COhep-thphysics.data-an
keywords cosmologicalgravitylatemodelstheoryviableaccelerationaccording
verification ladder T0 review T1 audit T2 compute T3 formal
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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 5 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Early- and late-time constraints on Wald-Gauss-Bonnet topological dark energy and implications for the $H_0$ and $S_8$ tensions

    gr-qc 2026-07 conditional novelty 6.0 of 10

    A joint CMB, BAO, and supernova fit mildly prefers a non-zero Wald-Gauss-Bonnet dark-energy term (~3σ with SH0ES included), raising H0 from 68.5 to 69.8 km/s/Mpc and easing the Hubble tension by ~0.9σ at the cost of a...

  2. Hubble tension in k-essence: Evidence for robust tension alleviation

    astro-ph.CO 2026-07 conditional novelty 5.0 of 10

    Dilaton and tachyon k-essence models robustly reduce Planck–late-Universe H0 tension to 0.14σ and 0.69σ without dataset-dependent fine-tuning of model parameters.

  3. Charged black hole solutions in $f(R,T)$ gravity coupled to nonlinear electrodynamics

    gr-qc 2024-11 conditional novelty 4.0 of 10

    The authors derive a family of charged black hole metrics in f(R,T)=R+βT gravity with Lagrangian L=f0+F+αF^p, show they have curvature singularities at the origin, and use the Sgr A* shadow to place weak upper bounds ...

  4. Cosmological solutions in teleparallel $F(T,B)$ gravity

    gr-qc 2024-11 conditional novelty 4.0 of 10

    A catalog of power-law F(T,B) gravity functions that solve teleparallel Robertson-Walker field equations for linear, quadratic, and scalar-field sources.

  5. Late Time Phenomena in $f(T,\mathcal{T})$ Gravity Framework: Role of $H_0$ Priors

    gr-qc 2024-11 conditional novelty 4.0 of 10

    An f(T,T) gravity model fitted to Pantheon+, BAO, and cosmic chronometer data yields a range of H0 posteriors that track the input priors, and predicts a growth rate about 9-11% below ΛCDM for two data combinations.

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