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Determining the core-collapse supernova explosion mechanism with current and future gravitational-wave observatories
Jade Powell, Alberto Iess, Miquel Llorens-Monteagudo +5
Gravitational waves are emitted from deep within a core-collapse supernova, which may enable us to determine the mechanism of the explosion from a gravitational-wave detection. Pre…
Self-consistent treatment of thermal effects in neutron-star post-mergers: observational implications for third-generation gravitational-wave detectors
Verónica Villa-Ortega, Ana Lorenzo-Medina, Juan Calderón Bustillo +4
We assess the impact of accurate, self-consistent modelling of thermal effects in neutron-star merger remnants in the context of third-generation gravitational-wave detectors. This…
Numerical evolutions of boson stars in Palatini gravity
Andreu Masó-Ferrando, Nicolas Sanchis-Gual, José A. Font +1
We investigate the time evolution of spherically symmetric boson stars in Palatini gravity through Numerical Relativity computations. Employing a novel approach th…
Revisiting the -Love- relations for superfluid neutron stars
Eneko Aranguren, José A. Font, Nicolas Sanchis-Gual +1
We study the tidal problem and the resulting -Love- approximate universal relations for rotating superfluid neutron stars in the Hartle-Thorne formalism. Superfluid stars are…
Assessment of a new sub-grid model for magnetohydrodynamical turbulence. II. Kelvin-Helmholtz instability
Miquel Miravet-Tenés, Pablo Cerdá-Durán, Martin Obergaulinger +1
The modelling of astrophysical systems such as binary neutron star mergers or the formation of magnetars from the collapse of massive stars involves the numerical evolution of magn…
Bayesian inference from gravitational waves in fast-rotating, core-collapse supernovae
Carlos Pastor-Marcos, Pablo Cerdá-Durán, Daniel Walker +4
Core-collapse supernovae (CCSNe) are prime candidates for gravitational-wave detectors. The analysis of their complex waveforms can potentially provide information on the physical…