10 citations · 21 across the 7 of their papers we have counts for
7 papers · 1 filter
Hyperon bulk viscosity effects in neutron-star inspirals
Elena M. Kantor, Mikhail E. Gusakov, Kirill Y. Kraav
The paper revisits the role of hyperon bulk viscosity during neutron-star inspiral. We find that hyperon bulk viscosity exerts only a minor influence on the gravitational-wave phas…
Instability windows of relativistic r-modes in stably stratified neutron stars with hyperonic cores
K. Y. Kraav, M. E. Gusakov, E. M. Kantor
(abridged) -modes are oscillations in rotating stars, primarily restored by the Coriolis force. These oscillations are the most susceptible to the Chandrasekhar-Friedman-Schutz…
Role of particle diffusion in shaping the gravitational wave signal from neutron star inspirals
Elena M. Kantor, Mikhail E. Gusakov, Kirill Y. Kraav
It is commonly believed that the dissipative properties of superdense matter play a negligible role in modeling gravitational waveforms from neutron star inspirals. This study aims…
Instability windows of relativistic r-modes
Kirill Y. Kraav, Mikhail E. Gusakov, Elena M. Kantor
The detectability of the gravitational-wave signal from -modes depends on the interplay between the amplification of the mode by the CFS instability and its damping due to dissi…
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…
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…