8 citations · 11 across the 6 of their papers we have counts for
6 papers
On the nature of oscillating modes of proto-neutron stars
Dimitra Tseneklidou, Alejandro Torres-Forne, Pablo Cerda-Duran +2
Newborn proto-neutron stars (PNS) are potential targets of gravitational wave asteroseismology, the study of the (inner) structure of stars via their oscillation modes. To prepare…
Towards asteroseismology of neutron stars with physics-informed neural networks
Dimitra Tseneklidou, Alejandro Torres-Forne, Pablo Cerda-Duran
The study of the gravitational wave signatures of neutron star oscillations may provide important information of their interior structure and Equation of State (EoS) at high densit…
Proto-neutron star oscillations including accretion flows
Dimitra Tseneklidou, Raimon Luna, Pablo Cerdá-Durán +1
The gravitational wave signature from core-collapse supernovae (CCSNe) is dominated by quadrupolar oscillation modes of the newly born proto-neutron star (PNS), and could be detect…
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…
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…
Relativistic magnetised perturbations: magnetic pressure vs magnetic tension
Dimitra Tseneklidou, Christos G. Tsagas, John D. Barrow
We study the linear evolution of magnetised cosmological perturbations in the post-recombination epoch. Using full general relativity and adopting the ideal magnetohydrodynamic app…