13 citations · 39 across the 6 of their papers we have counts for
7 papers
An efficient approach to resistive GRMHD simulations of binary neutron star mergers
Miquel Miravet-Tenés, Ian Hawke, Rahime Matur +1
Astrophysical plasmas are often highly conducting, but finite resistivity can nevertheless influence the evolution of strongly magnetised systems. Capturing these effects in genera…
Identifying thermal effects in neutron star merger remnants with model-agnostic waveform reconstructions and third-generation detectors
Miquel Miravet-Tenés, Davide Guerra, Milton Ruiz +2
We probe the intrinsic differences in simulated gravitational-wave signals from binary neutron star (BNS) mergers, arising from varying approaches to incorporating thermal effects…
Bayesian real-time classification of multi-messenger electromagnetic and gravitational-wave observations
Marina Berbel, Miquel Miravet-Tenés, Sushant Sharma Chaudhary +7
Because of the electromagnetic radiation produced during the merger, compact binary coalescences with neutron stars may result in multi-messenger observations. In order to follow u…
Prospects for the inference of inertial modes from hypermassive neutron stars with future gravitational-wave detectors
Miquel Miravet-Tenés, Florencia L. Castillo, Roberto De Pietri +2
Some recent, long-term numerical simulations of binary neutron star mergers have shown that the long-lived remnants produced in such mergers might be affected by convective instabi…
Assessment of a new sub-grid model for magneto-hydrodynamical turbulence. I. Magnetorotational instability
Miquel Miravet-Tenés, Pablo Cerdá-Durán, Martin Obergaulinger +1
Insufficient numerical resolution of grid-based, direct numerical simulations (DNS) hampers the development of instabilitydriven turbulence at small (unresolved) scales. As an alte…
Impact of ultralight bosonic dark matter on the dynamical bar-mode instability of rotating neutron stars
Fabrizio Di Giovanni, Nicolás Sanchis-Gual, Davide Guerra +3
We investigate the effects ultralight bosonic field dark matter may have on the dynamics of unstable differentially-rotating neutron stars prone to the bar-mode instability. To thi…
Fermion-axion stars: static solutions and dynamical stability
Fabrizio Di Giovanni, Davide Guerra, Simone Albanesi +2
We construct spherically-symmetric static solutions of the Einstein-Klein-Gordon-Euler system involving a complex scalar field governed by a periodic potential which emerges in mod…