Relaxation of the Angular Velocity of the Vela Pulsar within the Framework of General Relativity. Quark Model of a Neutron Star

Details Relaxation of the Angular Velocity of the Vela Pulsar within the Framework of General Relativity. Quark Model of a Neutron Star Relaxation of the Angular Velocity of the Vela Pulsar within the Framework of General Relativity. Quark Model of a Neutron Star

Oct 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000ap.....43..458h&link_type=abstract

Astrophysics (English translation of Astrofizika), v. 43, Issue 4, p. 458-462 (2000).

Astronomy and Astrophysics

Astrophysics

Scientific paper

A previously developed theory of the relaxation of a pulsar's angular velocity within the framework of general relativity is compared with observational data for the Vela pulsar on the basis of a quark model of a neutron star. The relative moments of inertia and the positions of relaxation regions are found. It is shown that the model of a neutron star containing normal quark matter is inconsistent with observations of the relaxation of pulsar angular velocity.

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