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G. Camelio

8 papers hereh-index 8154 citations10 works total

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • sole author1
  • first author6
  • last author1

Across the 8 of 8 papers where every author was matched, so the position is known.

fields
  • gr-qc4
  • astro-ph.HE3
  • nucl-th1

identity via Semantic Scholar / OpenAlex

activity
20172022
most citedSimulating bulk viscosity in neutron stars. II. Evolution in spherical symmetry

29 citations · 69 across the 5 of their papers we have counts for

collaborators
Showing astro-ph.HEShow all

3 papers · 1 filter

astro-ph.HE2020★ 28 cited

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…

astro-ph.HE2018

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…

astro-ph.HE2017

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…

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Not affiliated with arXiv. Researcher data from Semantic Scholar (ODC-BY) and OpenAlex.