The Physical Essence of Pulsar Glitch
classification
🌌 astro-ph.HE
hep-ph
keywords
neutronglitchmodelphasepulsarssuperfluidbehaviordipole
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Based on the magnetic dipole radiation from the 3P2 neutron superfluid vortices (3P2NSFV) in neutron stars, we propose a model of glitch for young pulsars by oscillation between B phase and A phase of 3P2 Neutron superfluid. The main behavior of glitches of pulsars may be naturally explained by our model.
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