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Modified gravity theories on a nutshell: Inflation, bounce and late-time evolution

TLDR
In this paper, the authors systematically review some standard issues and also the latest developments of modified gravity in cosmology, emphasizing on inflation, bouncing cosmology and late-time acceleration era.
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This article is published in Physics Reports.The article was published on 2017-06-02 and is currently open access. It has received 1950 citations till now. The article focuses on the topics: Gravitation & Dark energy.

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In the realm of the Hubble tension - a review of solutions

TL;DR: In this paper, the authors present a thorough review of recent Hubble constant estimates and a summary of the proposed theoretical solutions, including early or dynamical dark energy, neutrino interactions, interacting cosmologies, primordial magnetic fields, and modified gravity.
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Cosmology Intertwined: A Review of the Particle Physics, Astrophysics, and Cosmology Associated with the Cosmological Tensions and Anomalies

Elcio Abdalla, +202 more
TL;DR: In this paper , the authors focus on the 5.0σ tension between the Planck CMB estimate of the Hubble constant H0 and the SH0ES collaboration measurements and discuss the importance of trying to fit a full array of data with a single model.
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Extended gravity cosmography

TL;DR: In this paper, the success and the shortcomings of the ΛCDM model, based on cosmography, are discussed and a review of the model's performance is presented. But the model is not considered as a sort of a model-independent approach to tackle the dark energy/modified gravity problem.
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Teleparallel theories of gravity: illuminating a fully invariant approach

TL;DR: In this article, the role of the inertial spin connection in removing the spurious inertial effects within a given frame of reference is emphasized, leading to the construction of a fully invariant theory of teleparallel gravity and its generalizations.
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Tsallis holographic dark energy

TL;DR: In this paper, a new holographic dark energy (HDE) model was proposed for the Friedmann-Robertson-Walker (FRW) universe in which there is no interaction between the cosmos sectors.
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