activity
20062025
most citedJ-PAS: The Javalambre-Physics of the Accelerated Universe Astrophysical Survey

151 citations · 943 across the 27 of their papers we have counts for

collaborators

27 papers

astro-ph.CO2025

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 c…

hep-ph2025★ 4 cited

Fully-heavy tetraquarks in the vacuum and in a hot environment

Vinícius S. Silva, Cássio Pigozzo, Luciano M. Abreu

We study the thermal behavior of quarkonia and fully-heavy tetraquark states associated to the charmonium, bottomonium and bottom-charmonium mass spectra. The starting point is the…

astro-ph.CO2024★ 1 cited

Dark sector interactions in light of weak lensing data

M. Benetti, P. T. Z. Seidel, C. Pigozzo +3

The current observational tensions in the standard cosmological model have reinforced the research on dynamical dark energy, in particular on models with non-gravitational interact…

astro-ph.CO2024★ 19 cited

Testing the isotropy of cosmic acceleration with Pantheon+ and SH0ES: A cosmographic analysis

Carlos A. P. Bengaly, Cássio Pigozzo, Jailson S. Alcaniz

We use a recent Pantheon+SH0ES compilation of Type Ia Supernova distance measurements at low-redshift, i.e., , in order to investigate the directional depend…

astro-ph.GA2023

Active galactic nuclei and gravitational redshifts

N. D. Padilla, S. Carneiro, J. Chaves-Montero +4

Context: Gravitational redshift is a classical effect of Einstein's General Relativity, already measured in stars, quasars and clusters of galaxies. Aims: We here aim to identify t…

astro-ph.CO2023★ 12 cited

Testing the growth rate in homogeneous and inhomogeneous interacting vacuum models

H. A. Borges, C. Pigozzo, P. Hepp +2

In this work we consider a class of interacting vacuum corresponding to a generalised Chaplygin gas (gCg) cosmology. In particular we analyse two different scenarios at perturbatio…