Output energy in pulsars

Details Output energy in pulsars Output energy in pulsars

Aug 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986esasp.251..425s&link_type=abstract

In ESA Proceedings of the Joint Varenna-Abastumani International School and Workshop on Plasma Astrophysics p 425-427 (SEE N87-

Physics

Condensed Matter

Superconductivity

Electrohydrodynamics, Pulsars, Superconductivity, Magnetic Flux, Magnetohydrodynamic Flow, Stellar Cores, Vortices

Scientific paper

It has been shown, when angular velocity of pulsars decreases, the neutron vortices parallel to the axis of rotation move radially to the boundary between star nucleus and crust. This will decrease the length of proton vortices in star nucleus, therefore, the magnetic energy of these vortices must release on the edge of the "npe"-phase. The full energy output is of the order of 5×1028 - 5×1031erg/sec, and the energy release takes place mainly near the equatorial plane.

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