Pinning of proton vortices in the superfluid cores of neutron stars

Details Pinning of proton vortices in the superfluid cores of neutron stars Pinning of proton vortices in the superfluid cores of neutron stars

Aug 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991zhetf.100..353s&link_type=abstract

Zhurnal Eksperimental'noi i Teoreticheskoi Fiziki (ISSN 0044-4510), vol. 100, Aug. 1991, p. 353-362. In Russian.

Astronomy and Astrophysics

Astronomy

3

Neutron Stars, Pulsars, Radio Emission, Stellar Cores, Superfluidity, Radio Sources (Astronomy), Stellar Evolution, Stellar Magnetic Fields, Vortices

Scientific paper

The pinning of two classes of proton vortices is investigated and several astrophysical consequences of this are considered. It is shown that pinning of proton vortices associated with the residual and generated magnetic field occurs in the superfluid cores of neutron stars. The motion of pinned vortices results in an asymmetric release of energy at the boundary of the superfluid core, and this leads to the formation of two sources of pulsar radio wave emission.

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