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20242026
most citedCDM cosmology from a type-II minimally modified gravity

8 citations · 8 across the 1 of their papers we have counts for

collaborators

13 papers

astro-ph.CO20268 cited

CDM cosmology from a type-II minimally modified gravity

Özgür Akarsu, Antonio De Felice, Eleonora Di Valentino +5

We integrate CDM, a promising scenario for alleviating cosmological tensions, into VCDM, a type-II minimally modified gravity. This promotes the scenario to a fully pre…

gr-qc2025

Nonsingular black holes and spherically symmetric objects in nonlinear electrodynamics with a scalar field

Antonio De Felice, Shinji Tsujikawa

In general relativity with vector and scalar fields given by the Lagrangian , where is a Maxwell term and is a kinetic term of the scalar field , we s…

gr-qc2025

The non-minimal 3-form cosmology and the rise of the cuscuton

Antonio De Felice, Anamaria Hell

We consider the 3-form theory with non-minimal coupling to gravity in an expanding Universe. First, we assume that the background is homogeneous and isotropic, and that the three-f…

gr-qc2025

Unexplored regions in teleparallel gravity: Sign-changing dark energy density

Ozgur Akarsu, Bilal Bulduk, Antonio De Felice +2

While gravity has shown considerable potential in addressing cosmological tensions, we explore previously overlooked solution spaces that hold further promise. We examine th…

gr-qc2025

Instability of regular planar black holes in four dimensions arising from an infinite sum of curvature corrections

Antonio De Felice, Shinji Tsujikawa

In four-dimensional scalar-tensor theories derived via dimensional regularization with a conformal rescaling of the metric, we study the stability of planar black holes (BHs) whose…

gr-qc2025

Greybody factors of charged black holes with axion hair

Ratchaphat Nakarachinda, Petarpa Boonserm, Antonio De Felice +2

We study the greybody factor of charged hairy black holes (BHs) that arise due to the presence of an axion coupled to the electromagnetic field. Specifically, we consider spin-0 an…