116 citations · 750 across the 26 of their papers we have counts for
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Thermal evolution of neo-neutron stars. I: envelopes, Eddington luminosity phase and implications for GW170817
Mikhail V. Beznogov, Dany Page, Enrico Ramirez-Ruiz
A neo-neutron star is a hot neutron star that has just become transparent to neutrinos. In a core collapse supernova or accretion induced collapse of a white dwarf the neo-neutron…
Cooling of the Cassiopeia A neutron star and the effect of diffusive nuclear burning
Wynn C. G. Ho, M. J. P. Wijngaarden, Philip Chang +4
The study of how neutron stars cool over time can provide invaluable insights into fundamental physics such as the nuclear equation of state and superconductivity and superfluidity…
Diffusive nuclear burning in cooling simulations and application to new temperature data of the Cassiopeia A neutron star
M. J. P. Wijngaarden, Wynn C. G. Ho, Philip Chang +4
A critical relation in the study of neutron star cooling is the one between surface temperature and interior temperature. This relation is determined by the composition of the neut…