activity
20092023
most citedDetermining with Bayesian hyper-parameters

94 citations · 479 across the 18 of their papers we have counts for

collaborators

18 papers

astro-ph.CO2023★ 6 cited

Scrutinizing coupled vector dark energy in light of data

Wilmar Cardona, Jose L. Palacios-Córdoba, César A. Valenzuela-Toledo

Since current challenges faced by CDM might be hinting at new unravelled physics, here we investigate a plausible cosmological model where a vector field acts as source of dark…

astro-ph.CO2022★ 14 cited

Using machine learning to compress the matter transfer function

J. Bayron Orjuela-Quintana, Savvas Nesseris, Wilmar Cardona

The linear matter power spectrum connects theory with large scale structure observations in cosmology. Its scale dependence is entirely encoded in the matter transfer func…

astro-ph.CO2022★ 13 cited

Holographic energy density, dark energy sound speed, and tensions in cosmological parameters: and

Wilmar Cardona, M. A. Sabogal

Interesting discrepancies in cosmological parameters are challenging the success of the CDM model. Direct measurements of the Hubble constant using Cepheid variables and s…

astro-ph.CO2022★ 15 cited

Momentum transfer in the dark sector and lensing convergence in upcoming galaxy surveys

Wilmar Cardona, David Figueruelo

We investigated a cosmological model that allows a momentum transfer between dark matter and dark energy. The interaction in the dark sector mainly affects the behaviour of perturb…

astro-ph.CO2022

An effective fluid description of scalar-vector-tensor theories under the sub-horizon and quasi-static approximations

Wilmar Cardona, J. Bayron Orjuela-Quintana, César A. Valenzuela-Toledo

We consider scalar-vector-tensor (SVT) theories with second-order equations of motion and tensor propagation speed equivalent to the speed of light. Under the sub-horizon and the q…

astro-ph.CO2020★ 10 cited

Cosmological constraints with the Effective Fluid approach for Modified Gravity

Wilmar Cardona, Rubén Arjona, Alejandro Estrada +1

Cosmological constraints of Modified Gravity (MG) models are seldom carried out rigorously. First, even though general MG models evolve differently (i.e., background and perturbati…