http://arxiv.org/abs/1810.01743
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.
Q. Peng, J. Liu and C. Chou
Thu, 4 Oct 18
23/72
Comments: 2 figures. arXiv admin note: text overlap with arXiv:1207.0633, arXiv:1502.07062 by other authors
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