Abstract
ABSTRACT Many pulsars show sudden rotation jumps, glitches, superimposed to the gradual rotation down due to the continued loss of energy by radiation. A lot of models have been proposed to explain glitches. Most of the models are associated with layer structure of neutron stars. We try to investigate possibility of relationship between glitches of Crab pulsar and Einstein-de Haas effect. In the scenarios, spin polarization of neutron matter with Skyrme-type interactions forms a macroscopic spin angular momentum, and the Einstein-de Haas effect – transfer between the macroscopic spin and orbit angular momentum – gives rise to glitches of pulsars. It is shown that the scenario is in agreement with the observations of Crab pulsar on glitches and post-glitches relaxation.
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Schedule a callDisclaimer: 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.
