Astronomy and Astrophysics – Astrophysics
Scientific paper
Jan 1999
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999ap.....42...64h&link_type=abstract
Astrophysics, Volume 42, Issue 1, pp.64-72
Astronomy and Astrophysics
Astrophysics
Scientific paper
The dynamics of the rotation of a two-component system in a neutron star is considered within the framework of the general theory of relativity. Equations for the angular velocities of the normal and superfluid components are obtained in the W approximation. It is shown that the solutions of these equations can describe the relaxation of pulsar angular velocity after a glitch.
Hairapetian M. V.
Sedrakian David M.
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