Astronomy and Astrophysics – Astrophysics
Scientific paper
Jun 2006
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006chjaa...6..297p&link_type=abstract
Chinese Journal of Astronomy and Astrophysics, Volume 6, Issue 3, pp. 297-304 (2006).
Astronomy and Astrophysics
Astrophysics
3
Scientific paper
Considering neutron star heating by magnetic dipole radiation from 3PF2 superfluid neutron vortices inside the star, we propose a neutron phase oscillation model between the normal neutron Fermi fluid and the 3PF2 superfluid neutron vortices at the transition temperature of Ttrans = (2-3)×108 K. With this model we can qualitatively explain most of the observations on pulsar glitches up to date.
Chou Chih-kang
Luo Zhi-Quan
Peng Qiu-he
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