79 citations · 211 across the 9 of their papers we have counts for
9 papers
Modeling Neutron Star Matter in the Age of Multimessenger Astrophysics
Omar Benhar, Alessandro Lovato, Giovanni Camelio
The interpretation of the available and forthcoming data obtained from multimessenger astrophysical observations -- potentially providing unprecedented access to neutron star prope…
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…
Axisymmetric models for neutron star merger remnants with realistic thermal and rotational profiles
Giovanni Camelio, Tim Dietrich, Stephan Rosswog +1
Merging neutron stars are expected to produce hot, metastable remnants in rapid differential rotation, which subsequently cool and evolve into rigidly rotating neutron stars or col…
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…
Disk formation in the collapse of supramassive neutron stars
Giovanni Camelio, Tim Dietrich, Stephan Rosswog
Short gamma-ray bursts (sGRBs) show a large diversity in their properties. This suggests that the observed phenomenon can be caused by different "central engines" or that the engin…
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…
Evolution of a proto-neutron star with a nuclear many-body equation of state: Neutrino luminosity and gravitational wave frequencies
Giovanni Camelio, Alessandro Lovato, Leonardo Gualtieri +3
In a core-collapse supernova, a huge amount of energy is released in the Kelvin-Helmholtz phase subsequent to the explosion, when the proto-neutron star cools and deleptonizes as i…
On the origin of intrinsic alignment in cosmic shear measurements: an analytic argument
Giovanni Camelio, Marco Lombardi
Galaxy intrinsic alignment can be a severe source of error in weak-lensing studies. The problem has been widely studied by numerical simulations and with heuristic models, but with…