Author: sylvia
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Time dependent signatures of core-collapse supernova neutrinos at HALO
We calculate the response of a lead-based detector, such as the Helium and Lead Observatory (HALO) or its planned upgrade HALO-1kt to a galactic core-collapse supernova. We pay particular attention […]
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Particle-in-cell Simulation of the Neutrino Fast Flavor Instability
Neutrinos drive core-collapse supernovae, launch outflows from neutron star merger accretion disks, and set the ratio of protons to neutrons in ejecta from both systems that generate heavy elements in […]
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Mapping dynamical ejecta and disk masses from numerical relativity simulations of neutron star mergers
We present fitting formulae for the dynamical ejecta properties and remnant disk masses from a large sample of numerical relativity simulations. The considered data include some of the latest simulations […]
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Updated universal relations for tidal deformabilities of neutron stars from phenomenological equations of state
Equation of state (EOS) insensitive relations, so-called universal relations, between the neutron star (NS) compactness, its multipolar tidal deformability coefficients, and between the tidal parameters for binary systems are essential […]