most citedPhase transitions in neutron stars and their links to gravitational waves

68 citations · 153 across the 5 of their papers we have counts for

collaborators

6 papers

nucl-th20201 cited

Non-local quark models for description of dense matter in the cores of neutron stars

German Malfatti

This thesis work focuses on studying the possible existence of phase transitions in the immediate compact remnants of core collapse supernova, neutron stars, and the theoretical mo…

astro-ph.HE2020

Hybrid stars with sequential phase transitions: the emergence of the g mode

M. C. Rodriguez, I. F. Ranea-Sandoval, M. Mariani +3

Neutron stars are the densest objects in the Universe, with and km, and the equation of state associated to their internal composition is still u…

astro-ph.HE202063 cited

Delta baryons and diquark formation in the cores of neutron stars

German Malfatti, Milva G. Orsaria, Ignacio F. Ranea-Sandoval +2

We investigate the hadron-quark phase transition in cold neutron stars in light of (i) the observed limits on the maximum-mass of heavy pulsars, (ii) constraints on the tidal prope…

nucl-th20191 cited

Phases of Hadron-Quark Matter in (Proto) Neutron Stars

F. Weber, D. Farrell, W. M. Spinella +4

In the first part of this paper, we investigate the possible existence of a structured hadron-quark mixed phase in the cores of neutron stars. This phase, referred to as the hadron…

astro-ph.HE201968 cited

Phase transitions in neutron stars and their links to gravitational waves

Milva G. Orsaria, Germán Malfatti, Mauro Mariani +6

The recent direct observation of gravitational wave event and its signal has opened up a new window to study neutron stars and heralds a new era of Astronom…

nucl-th201920 cited

Effects of Hadron-Quark Phase Transitions in Hybrid Stars within the NJL Model

Ignacio Francisco Ranea-Sandoval, Milva Gabriela Orsaria, Germán Malfatti +4

We study local and non-local Polyakov Nambu-Jona-Lasinio models and analyze their respective phase transition diagram. We construct hybrid stars using the zero temperature limit of…