3 papers
astro-ph1999
A simple model of cooling neutron stars with superfluid cores: comparison with observations
K. P. Levenfish, Yu. A. Shibanov, D. G. Yakovlev
Cooling of neutron stars (NSs) with superfluid cores is simulated taking into account neutrino emission produced by Cooper pairing of nucleons. The critical temperatures of neutron…
astro-ph1998
Equation of state and opacities for hydrogen atmospheres of strongly magnetized cooling neutron stars
A. Y. Potekhin, Yu. A. Shibanov, J. Ventura
We study partially ionized hydrogen plasma at temperatures T = 10^{5.5}-10^{6.5} K and magnetic fields B = 10^{12}-10^{13} G, typical of photospheres of isolated neutron stars. We…
astro-ph1996
Model neutron star atmospheres with low magnetic fields. 1. Atmospheres in radiative equilibrium
V. E. Zavlin, G. G. Pavlov, Yu. A. Shibanov
We present a detailed investigation of neutron star atmospheres with low magnetic fields, G, which do not affect opacities and equation of state of the atmosphe…