3 papers
astro-ph.HE2021
Diffusion as a leading dissipative mechanism in superconducting neutron stars
K. Y. Kraav, M. E. Gusakov, E. M. Kantor
Despite the fact that different particle species can diffuse with respect to each other in neutron star (NS) cores, the effect of particle diffusion on various phenomena associated…
astro-ph.HE2018
Precession and glitches in the framework of three-component model of neutron star
D. P. Barsukov, O. A. Goglichidze, K. Y. Kraav +1
We consider the pulsar rotation assuming that the neutron star consists of crust component (which rotation is observed) and two core components. One of the core components contains…
astro-ph.HE2017
The influence of small-scale magnetic field on the evolution of inclination angle and precession damping in the framework of 3-component model of neutron star
K. Y. Kraav, M. V. Vorontsov, D. P. Barsukov
The evolution of inclination angle and precession damping of radio pulsars is considered. It is assumed that the neutron star consists of 3 "freely" rotating components: the crust…