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20082022
most citedDynamical dark energy after Planck CMB final release and tension

100 citations · 430 across the 14 of their papers we have counts for

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Showing astro-ph.COShow all

8 papers · 1 filter

astro-ph.CO2022★ 5 cited

Equality scale-based and sound horizon-based analysis of the Hubble tension

Zhihuan Zhou, Yuhao Mu, Gang Liu +2

The Hubble horizon at matter-radiation equality () and the sound horizon at the last scattering surface () provides interesting consistency check for th…

astro-ph.CO2021★ 100 cited

Dynamical dark energy after Planck CMB final release and tension

Weiqiang Yang, Eleonora Di Valentino, Supriya Pan +2

In this article we compare a variety of well known dynamical dark energy models using the cosmic microwave background measurements from the 2018 Planck legacy and 2015 Planck data…

astro-ph.CO2019

Challenging bulk viscous unified scenarios with cosmological observations

Weiqiang Yang, Supriya Pan, Eleonora Di Valentino +2

In a spatially flat Friedmann-Lemaître-Robertson-Walker universe, we investigate a unified cosmic fluid scenario endowed with bulk viscosity in which the coefficient of the bulk vi…

astro-ph.CO2016

Cosmic constraint on massive neutrinos in viable f(R) gravity with producing LCDM background expansion

Jianbo Lu, Molin Liu, Yabo Wu +2

Tensions between several cosmic observations were found recently, such as the inconsistent values of (or ) were indicated by the different cosmic observations. Intro…

astro-ph.CO2011★ 54 cited

Combined constraints on modified Chaplygin gas model from cosmological observed data: Markov Chain Monte Carlo approach

Jianbo Lu, Lixin Xu, Yabo Wu +1

We use the Markov Chain Monte Carlo method to investigate a global constraints on the modified Chaplygin gas (MCG) model as the unification of dark matter and dark energy from the…

astro-ph.CO2009★ 56 cited

Generalized Holographic and Ricci Dark Energy Models

Lixin Xu, Jianbo Lu, Wenbo Li

In this paper, we consider generalized holographic and Ricci dark energy models where the energy densities are given as and $ρ_{h}=3c^2M^{2}_{pl}H^2…