28 citations · 31 across the 2 of their papers we have counts for
4 papers
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…