activity
19992024
most citedIn the Realm of the Hubble tension a Review of Solutions

2k citations · 14.6k across the 169 of their papers we have counts for

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Showing 2018Show all

10 papers · 1 filter

astro-ph.CO2018★ 54 cited

Future Constraints on Dynamical Dark-Energy using Gravitational-Wave Standard Sirens

Minghui Du, Weiqiang Yang, Lixin Xu +2

The detection of gravitational waves (GW) by the LIGO and Virgo collaborations offers a whole new range of possible tests and opens up a new window which may shed light on the natu…

astro-ph.CO2018★ 20 cited

Screenings in Modified Gravity: a perturbative approach

Alejandro Aviles, Jorge L. Cervantes-Cota, David F. Mota

We present a formalism to study screening mechanisms in modified theories of gravity via perturbative methods in different cosmological scenarios. We consider Einstein frame posed…

astro-ph.CO2018★ 20 cited

Halo collapse: virialization by shear and rotation in dynamical dark-energy models. Effects on weak-lensing peaks

Francesco Pace, Carlo Schimd, David F. Mota +1

The evolution of the virial overdensity for CDM and seven dynamical dark-energy models is investigated in the extended spherical collapse model (SCM). Here the vir…

astro-ph.CO2018★ 75 cited

Cosmological constraints on parametrized interacting dark energy

R. von Marttens, L. Casarini, D. F. Mota +1

We reconsider the dynamics of the Universe in the presence of interactions in the cosmological dark sector. A class of interacting models is introduced via a real function $f\left(…

astro-ph.CO2018★ 10 cited

Probing modified gravity in cosmic filaments

Alex Ho, Max Gronke, Bridget Falck +1

Multiple modifications of general relativity (GR) have been proposed in the literature in order to understand the nature of the accelerated expansion of the Universe. However, thus…

astro-ph.CO2018★ 346 cited

Tale of stable interacting dark energy, observational signatures, and the tension

Weiqiang Yang, Supriya Pan, Eleonora Di Valentino +3

We investigate the observational consequences of a novel class of stable interacting dark energy (IDE) models, featuring interactions between dark matter (DM) and dark energy (DE).…