gluon condensate in pulsar cores explain pulsar glitches ? Raka
نویسنده
چکیده
Making use of the possibility that gluon condensate can be formed in neutron star core, we study the vortex pinning force between the crust and the interior of the neutron star. Our estimations indicate an increase in pinning strength with the age of the neutron star. This helps in explaining observed pulsar glitches and removes some difficulties faced by vortex creep model.
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تاریخ انتشار 1998