The next galactic core-collapse supernova (CCSN) has already exploded, and its
electromagnetic (EM) waves, neutrinos, and gravitational waves (GWs) may arrive at any …

The fine-structure constant and the electron mass in string theory are determined by the
values of scalar fields called moduli. If the dark matter takes on the form of such a light …

In this paper, we review the most common descriptions for the first-order phase transition to
deconfined quark matter in the core of neutron stars. We also present a new description of …

SCHENBERG is a resonant-mass gravitational wave detector built in Brazil. Its spherical
antenna, weighting 1.15 t, is connected to the outside world by a suspension system whose …

Estudos em diversos países, no âmbito do projeto Rose, avaliaram o interesse de
estudantes por temas científicos. Em geral, verificou-se que os temas relacionados a …

The present day gravitational wave (GW) detectors strive to detect the length variation,
which, owing to the smallness of the metric perturbation∼ h, is an extremely small length …

This article is an account of the work done in the Mario Schenberg gravitational wave
antenna up to date, focusing mainly in the participation of the Laboratório de Estado Sólido …

The main purpose of this study is to review the Schenberg resonant antenna transfer
function and to recalculate the antenna design strain sensitivity for gravitational waves. We …

Owing to the extreme smallness of any noncommutative scale that may exist in nature, both
in the spatial and momentum sector of the quantum phase space, a credible possibility of …

We report the plausibility of using quantum mechanical transitions, induced by the combined
effect of gravitational waves (GWs) and noncommutative (NC) structure of space, among the …