arXiv subjects

L. S. Brito

Publications and source records attributed to L. S. Brito.

3 recordsLinked to original sources

arXiv2026

Cosmological Constraints on $Λ$(t)CDM Models

Problems with the concordance cosmology $Λ$CDM as the cosmological constant problem, coincidence problems and Hubble tension has led to many proposed alternatives, as the $Λ(t)$CDM, where the now called $Λ$ cosmological term is allowed to vary due to an interaction with pressureless matter. Here, we analyze one class of these proposals, namely, $Λ=α'a^{-2}+βH^2+λ_*$, based on dimensional arguments. Using SNe Ia, cosmic chronometers data plus constraints on $H_0$ from SH0ES and Planck satellite, we constrain the free parameters of this class of models. By using the Planck prior over $H_0$, we conclude that the $λ_*$ term can not be discarded by this analysis, thereby disfavouring models only with the time-variable terms. The SH0ES prior over $H_0$ has an weak evidence in this direction. The subclasses of models with $α'=0$ and with $β=0$ can not be discarded by this analysis. Finally, by using distance priors from CMB, the $Λ$ time-dependence was quite restricted.

astro-ph.CO↗

arXiv2025

The rings of (2060) Chiron: Evidence of an evolving system

The centaur (2060) Chiron has long been a candidate for hosting material in orbit, based on occultation and photometric and spectroscopic data. Here, we present a multichord stellar occultation observed on 2023 September 10 UT that reveals new and complex structures surrounding Chiron. High-cadence light curves show multiple secondary events that are best explained (when compared with a multishell interpretation) with a system of three confined rings located at average radii of 273, 325, and 438 km, the outermost of which lies beyond Chiron's Roche limit. The rings appear coplanar, with a mean pole orientation of λ = 151° +/- 4° and \b{eta} = 20° +/- 6°. A broader, disklike structure extends from about 200 to 800 km, and a newly detected faint feature is observed at ~1380 km. Chiron thus appears as the fourth small solar system body known for hosting a ring system. Comparisons with previous occultation events that have occurred since 1994 show that these features are not permanent. With these observations, we may witness for the first time the ongoing formation and evolution of a ring system.

astro-ph.EP↗

arXiv2025

Can decaying vacuum solve the H_0 Tension?

In the present work we analyze two different models of interaction between dark energy and dark matter, also known as vacuum decay models or $Λ(t)$CDM models. In both models, when the $H_0$ parameter is constrained by the Planck distance priors, its value is compatible with a higher value of $H_0$, in agreement with SH0ES data, while simultaneously reducing the values of $Ω_m$ and $Ω_b$. In both models, we find $H_0=73.1\pm0.86$ at 68\% c.l. by combining Planck+SH0ES data. We also find the decay parameter to be $\varepsilon=0.0197^{+0.0032}_{-0.0027}$ for one model and $\varepsilon=0.0203\pm0.0034$ for the other one. From these analyses, a noninteracting model is excluded at least at $6σ$ c.l.! This shows that these types of models are promising in solving or at least alleviating the $H_0$ tension problem. Our analysis also shows a preference for the decay of vacuum into dark matter, in agreement to thermodynamic analyses.

astro-ph.CO↗