collaborators

13 papers

astro-ph.CO2026

Coupled quintessence from an axion dark sector

Rayff de Souza, Edmund J. Copeland, Jailson Alcaniz

Recent observational data arising from the DESI collaboration has hinted at a possible departure from the standard CDM cosmological model, preferring instead the presence of a d…

astro-ph.CO2026

Revisiting the CMB homogeneity scale: low multipoles removal effect and extragalactic foreground masking

Xiaoyun Shao, Facundo Toscano, Diego Garcia Lambas +5

The Cosmic Microwave Background (CMB) reaches homogeneity at relatively modest angular scales compared to the expectation of the standard CDM model revealing an important chall…

astro-ph.CO2026

Hubble tension and small-scale inhomogeneities on light propagation

Lucila Kraiselburd, Cassio Pigozzo, Susana J. Landau +1

Context. A major observational challenge within the standard cosmological framework is the Hubble tension, a statistically significant () disagreement between the Hubble…

astro-ph.CO2025

A model-independent assessment of the late-time dark energy density evolution

Rayff de Souza, Agripino Sousa-Neto, Javier E. González +1

Combined measurements of Baryon Acoustic Oscillations (BAO) from the Dark Energy Spectroscopic Survey (DESI), the Cosmic Microwave Background (CMB) and Type Ia Supernovae (SN Ia),…

astro-ph.CO2025

Thawing quintessence and transient cosmic acceleration in light of DESI

Rayff de Souza, Gabriel Rodrigues, Jailson Alcaniz

Recent analysis of the DESI Collaboration challenges the -Cold Dark Matter (CDM) model, suggesting evidence for a dynamic dark energy. These results are obtained in the con…

astro-ph.CO2025

Cosmography with DESI DR2 and SN data

Gabriel Rodrigues, Rayff de Souza, Jailson Alcaniz

In this paper, we present a kinematic analysis of the Universe's expansion history using cosmography, with a particular emphasis on the jerk parameter , which is equal to one…