The Physical Essence of Pulsar Glitch
classification
🌌 astro-ph.HE
hep-ph
keywords
neutronglitchmodelphasepulsarssuperfluidbehaviordipole
pith:IU72L2BE Add to your LaTeX paper
What is a Pith Number?\usepackage{pith}
\pithnumber{IU72L2BE}
Prints a linked pith:IU72L2BE badge after your title and writes the identifier into PDF metadata. Compiles on arXiv with no extra files. Learn more
read the original abstract
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.
This paper has not been read by Pith yet.
discussion (0)
Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.