12 citations · 25 across the 7 of their papers we have counts for
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Neutron contribution to the force on a proton vortex in superconducting neutron-star matter
Oleg A. Goglichidze, Mikhail E. Gusakov
We investigate the forces acting on a proton vortex in superconducting neutron-star matter composed of neutrons, protons, and electrons, accounting for Fermi-liquid interactions in…
Non-purely transverse Magnus force in superconducting neutron stars
Oleg A. Goglichidze, Mikhail E. Gusakov
The force acting on a proton vortex in extreme type-II superconducting neutron star matter is studied in the limit of vanishing temperature. A detailed analysis is presented on how…
Diffusion in superfluid Fermi mixtures: General formalism
Oleg A. Goglichidze, Mikhail E. Gusakov
With neutron star applications in mind, we developed a theory of diffusion in mixtures of superfluid, strongly interacting Fermi liquids. By employing the Landau theory of Fermi li…
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…
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 spin evolution of neutron stars with the superfluid core
D. P. Barsukov, O. A. Goglichidze, A. I. Tsygan
We investigate the neutron stars spin evolution (breaking, inclination angle evolution and radiative precession), taking into account the superfluidity of the neutrons in the star…