79 citations · 211 across the 9 of their papers we have counts for
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Simulating bulk viscosity in neutron stars. II. Evolution in spherical symmetry
Giovanni Camelio, Lorenzo Gavassino, Marco Antonelli +2
Out-of-equilibrium reactions between different particle species are the main processes contributing to bulk viscosity in neutron stars. In this work, we numerically compare three d…
Simulating bulk viscosity in neutron stars. I. Formalism
Giovanni Camelio, Lorenzo Gavassino, Marco Antonelli +2
The faithful inclusion of the effects of bulk viscosity induced by the presence of chemical reactions is an important issue for simulations of core-collapse supernovae, binary neut…
Rotating neutron stars with non-barotropic thermal profile
Giovanni Camelio, Tim Dietrich, Miguel Marques +1
Neutron stars provide an excellent laboratory for physics under the most extreme conditions. Up to now, models of axisymmetric, stationary, differentially rotating neutron stars we…
Early evolution of newly born proto-neutron stars
Giovanni Camelio
A proto-neutron star (PNS) is the first phase of life of a neutron star, and is likely to origin from a core-collapse supernova. After about 200 ms from core-collapse, the PNS evol…