Superfluidity and magnetic fields of pulsars.

Details Superfluidity and magnetic fields of pulsars. Superfluidity and magnetic fields of pulsars.

Jul 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991usfin.161....3s&link_type=abstract

Usp. Fiz. Nauk, Vol. 161, No. 7, p. 3 - 40

Physics

13

Scientific paper

A review of the modern state of superfluidity theory in pulsars is presented. Superfluidity of hadronic matter in the neutron stars is considered. It is shown that a strong interaction between neutron and proton condensates leads to the drag current of superconducting protons and to the generation of the strong magnetic field B = 1012Gs, which is parallel to the axis of rotation and constant in time. The value of this field depends on microscopic parameters of superfluid hadrons. The authors discuss the models explaining the origin of glitches and the postglitch relaxation. They calculate the coupling time between neutron superfluid and the right crust of the neutron star.

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