activity
20122026
most citedRelic Neutrinos, thermal axions and cosmology in early 2014

109 citations · 773 across the 30 of their papers we have counts for

collaborators

30 papers

astro-ph.CO20268 cited

Revisiting CPL with sign-switching density: To cross or not to cross the NECB

Mine Gökçen, Özgür Akarsu, Eleonora Di Valentino

Recent DESI DR2 BAO measurements, when combined with CMB and SNeIa data, exhibit a - preference for dynamical dark energy (DE) described by the CPL-parametrized equatio…

astro-ph.CO2025

The Serendipitous Axiodilaton: A Self-Consistent Recombination-Era Solution to the Hubble Tension

Adam Smith, Maria Mylova, Carsten van de Bruck +2

Axio-dilaton cosmology provides a minimal benchmark model for both Dark Matter (DM) and Dark Energy (DE) that is well motivated by fundamental physics. The axion and dilaton arise…

astro-ph.CO202510 cited

Decay of quintessence into dark matter: mitigating the Hubble tension?

Giovanni Montani, Luis A. Escamilla, Nakia Carlevaro +1

We propose a revised cosmological scenario that extends the Cold Dark Matter (CDM) framework by incorporating metric gravity in the Jordan frame. In this model, the d…

gr-qc202517 cited

III. Interacting Dark Energy: Summary of Models, Pathologies, and Constraints

Marcel van der Westhuizen, Amare Abebe, Eleonora Di Valentino

We present an overview of the main results from our two companion papers that are relevant for observational constraints on interacting dark energy (IDE) models. We provide analyti…

gr-qc20258 cited

I. Linear Interacting Dark Energy: Analytical Solutions and Theoretical Pathologies

Marcel van der Westhuizen, Amare Abebe, Eleonora Di Valentino

Interacting dark energy (IDE) models, in which dark matter (DM) and dark energy (DE) exchange energy through a non-gravitational interaction, have long been proposed as candidates…

gr-qc20259 cited

II. Non-Linear Interacting Dark Energy: Analytical Solutions and Theoretical Pathologies

Marcel van der Westhuizen, Amare Abebe, Eleonora Di Valentino

We investigate interacting dark energy (IDE) models with phenomenological, non-linear interaction kernels , specifically $Q_{1}=3Hδ\left(\frac{ρ_{\rm dm}ρ_{\rm de}}{ρ_{\rm dm}+ρ…