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Proper way to spatially decompose the gravitational-wave origin in stellar collapse simulations
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Gmunu: paralleled, grid-adaptive, general-relativistic magnetohydrodynamics in curvilinear geometries in dynamical space–times
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Black hole-neutron star simulations with the
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Equation of State and Progenitor Dependence of Stellar-mass Black Hole Formation
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Magnetorotational core collapse of possible GRB progenitors – I. Explosion mechanisms
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Towards asteroseismology of core-collapse supernovae with gravitational wave observations – II. Inclusion of space–time perturbations
Alejandro Torres-Forné, Pablo Cerdá-Durán, Andrea Passamonti, Martin Obergaulinger and José A Font Monthly Notices of the Royal Astronomical Society 482(3) 3967 (2019) https://doi.org/10.1093/mnras/sty2854
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Three-dimensional general-relativistic hydrodynamic simulations of binary neutron star coalescence and stellar collapse with multipatch grids
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Correlated gravitational wave and neutrino signals from general-relativistic rapidly rotating iron core collapse
A NEW MULTI-DIMENSIONAL GENERAL RELATIVISTIC NEUTRINO HYDRODYNAMICS CODE FOR CORE-COLLAPSE SUPERNOVAE. II. RELATIVISTIC EXPLOSION MODELS OF CORE-COLLAPSE SUPERNOVAE
Magnetoelastic oscillations of neutron stars with dipolar magnetic fields
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Discontinuous Galerkin methods for general-relativistic hydrodynamics: Formulation and application to spherically symmetric spacetimes
Relativistic simulations of the phase-transition-induced collapse of neutron stars
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