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researcher

Ignacio F. Ranea‐Sandoval

4 papers here

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

author position
  • first author1
  • middle author2
  • last author1

Across the 4 of 4 papers where every author was matched, so the position is known.

fields
  • astro-ph.HE3
  • nucl-th1
ORCID 0000-0002-9071-4634

identity via Semantic Scholar / OpenAlex

activity
20192024
most citedHot quark matter and (proto-) neutron stars

62 citations · 125 across the 4 of their papers we have counts for

collaborators

3 papers

astro-ph.HE2023★ 23 cited

Three approaches for the classification of protoneutron star oscillation modes

M. C. Rodriguez, Ignacio F. Ranea-Sandoval, C. Chirenti +1

The future detection of gravitational waves (GWs) from a galactic core-collapse supernova will provide information on the physics inside protoneutron stars (PNS). In this work, we…

astro-ph.HE2022★ 17 cited

Breaking of universal relationships of axial wI-modes in hybrid stars: rapid and slow hadron-quark conversion scenarios

Ignacio F. Ranea-Sandoval, Octavio M. Guilera, Mauro Mariani +1

Multi-messenger astronomy with gravitational waves is a blooming area whose limits are not clear. After the first detection of binary black hole merger and the famous event GW17081…

nucl-th2019★ 62 cited

Hot quark matter and (proto-) neutron stars

G. Malfatti, M. Orsaria, G. A. Contrera +2

In part one of this paper, we use a non-local extension of the 3-flavor Polyakov-Nambu-Jona-Lasinio model, which takes into account flavor-mixing, momentum dependent quark masses,…

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