activity
19982004
most citedThermal states of coldest and hottest neutron stars in soft X-ray transients

69 citations · 132 across the 5 of their papers we have counts for

collaborators

9 papers

astro-ph2004

Cooling of neutron stars: effects of accreted envelopes, magnetic field and crustal superfluidity

G. Chabrier, A. Y. Potekhin, D. G. Yakovlev

We briefly review recent theoretical studies of the effects of accreted envelopes, magnetic fields and crustal superfluidity on the cooling of neutron stars. These effects are espe…

astro-ph200369 cited

Thermal states of coldest and hottest neutron stars in soft X-ray transients

D. G. Yakovlev, K. P. Levenfish, A. Y. Potekhin +2

We calculate the thermal structure and quiescent thermal luminosity of accreting neutron stars (warmed by deep crustal heating in accreted matter) in soft X-ray transients (SXTs).…

astro-ph200362 cited

Neutron star cooling: Theoretical aspects and observational constraints

D. G. Yakovlev, O. Y. Gnedin, A. D. Kaminker +2

The cooling theory of isolated neutron stars is reviewed. The main cooling regulators are discussed, first of all, operation of direct Urca process (or similar processes in exotic…

astro-ph2002

Pycnonuclear burning and accreting neutron stars

D. G. Yakovlev, K. P. Levenfish

We outline the phenomenon of deep crustal heating in transiently accreting neutron stars. It is produced by nuclear transformations (mostly, by pycnonuclear reactions) in accreted…

astro-ph20021 cited

Cooling of superfluid neutron stars with muons

M. Bejger, D. G. Yakovlev, O. Y. Gnedin

We extend our modeling of cooling of superfluid neutron stars by including the production of muons in the core, in addition to neutrons, protons, and electrons. The results are con…

astro-ph2002

Cooling of Superfluid Neutron Stars

D. G. Yakovlev, O. Y. Gnedin, A. D. Kaminker +1

Cooling of neutron stars (NSs) with the cores composed of neutrons, protons, and electrons is analyzed. The main cooling regulators are discussed: opening of direct Urca process in…