36 citations · 64 across the 9 of their papers we have counts for
9 papers
The influence of small scale magnetic field on the heating of J0250+5854 polar cap
D. P. Barsukov, M. V. Vorontsov, I. K. Morozov
The influence of surface small scale magnetic field on the heating of PSR J0250+5854 polar cap is considered. It is assumed that polar cap is heated only by reverse positrons, acce…
Glitches in neutron stars with magnetically decoupled core
O. A. Goglichidze, D. P. Barsukov
The magnetically decoupled core model was proposed earlier as a way to solve the problem of inconsistency between the neutron star long-period precession and superfluid vortex pinn…
A possible way to reconcile long-period precession with vortex pinning in neutron stars
O. A. Goglichidze, D. P. Barsukov
We propose a possible way to solve the problem of inconsistency between the neutron star long-period precession and superfluid vortex pinning, which is the basis of the most succes…
Absorption of Photons from Distant Gamma-Ray Sources
A. N. Popov, D. P. Barsukov, A. V. Ivanchik
Being the largest gravitationally bound structures in the Universe, galaxy clusters are huge reservoirs of photons generated by the bremsstrahlung of a hot cluster gas. We consider…
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…
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…