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GW170817: Joint Constraint on the Neutron Star Equation of State from Multimessenger Observations
David Radice, Albino Perego, Francesco Zappa +1
Gravitational waves detected from the binary neutron star (NS) merger GW170817 constrained the NS equation of state by placing an upper bound on certain parameters describing the b…
Gravitational-wave luminosity of binary neutron stars mergers
Francesco Zappa, Sebastiano Bernuzzi, David Radice +2
We study the gravitational-wave peak luminosity and radiated energy of quasicircular neutron star mergers using a large sample of numerical relativity simulations with different bi…
AT2017gfo: an anisotropic and three-component kilonova counterpart of GW170817
Albino Perego, David Radice, Sebastiano Bernuzzi
The detection of a kilo/macronova electromagnetic counterpart (AT2017gfo) of the first gravitational wave signal compatible with the merger of two neutron stars (GW170817) has conf…
Turbulence in Core-Collapse Supernovae
David Radice, Ernazar Abdikamalov, Christian D. Ott +3
Multidimensional simulations show that non-radial, turbulent, fluid motion is a fundamental component of the core-collapse supernova (CCSN) explosion mechanism. Neutrino-driven con…
The impact of vorticity waves on the shock dynamics in core-collapse supernovae
Cesar Huete, Ernazar Abdikamalov, David Radice
Convective perturbations arising from nuclear shell burning can play an important role in propelling neutrino-driven core-collapse supernova explosions. In this work, we analyze th…
General-Relativistic Large-Eddy Simulations of Binary Neutron Star Mergers
David Radice
The flow inside remnants of binary neutron star (NS) mergers is expected to be turbulent, because of magnetohydrodynamics instability activated at scales too small to be resolved i…