Abstract
The motion of the neutron-proton vortex system in neutron stars is examined taking pinning and depinning of the vortices into account. The relaxation solution of the equations for the dynamics of pulsar rotation after glitches is compared with observational data on the Vela pulsar. It is shown that the angular rotation relaxation parameters are related both to the appearance of a “density wave” of neutron vortices during a glitch and to features of the motion of the vortices between successive glitches.
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Disclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.