116 citations · 302 across the 5 of their papers we have counts for
10 papers
Heat blanketing envelopes of neutron stars
M. V. Beznogov, A. Y. Potekhin, D. G. Yakovlev
Near the surface of any neutron star there is a thin heat blanketing envelope that produces substantial thermal insulation of warm neutron star interiors and that relates the inter…
Thermal luminosities of cooling neutron stars
A. Y. Potekhin, D. A. Zyuzin, D. G. Yakovlev +2
Ages and thermal luminosities of neutron stars, inferred from observations, can be interpreted with the aid of the neutron star cooling theory to gain information on the properties…
NS 1987A in SN 1987A
Dany Page, Mikhail V. Beznogov, Iván Garibay +3
The possible detection of a compact object in the remnant of SN 1987A presents an unprecedented opportunity to follow its early evolution. The suspected detection stems from an exc…
The effect of diffusive nuclear burning in neutron star envelopes on cooling in accreting systems
M. J. P Wijngaarden, Wynn C. G. Ho, Philip Chang +6
Valuable information about the neutron star interior can be obtained by comparing observations of thermal radiation from a cooling neutron star crust with theoretical models. Nucle…
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…