Superfluidity in neutron stars

Details Superfluidity in neutron stars Superfluidity in neutron stars

Jul 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985natur.316...27p&link_type=abstract

Nature (ISSN 0028-0836), vol. 316, July 4, 1985, p. 27-32.

Astronomy and Astrophysics

Astrophysics

188

Neutron Stars, Stellar Structure, Superfluidity, Protons, Pulsars, Stellar Cores, Stellar Mass Accretion, Stellar Rotation, Vortices

Scientific paper

Astrophysical evidence is reviewed for the existence of at least three distinct superfluids inside neutron stars from the observed relaxation of the rotation and spin-down rates of the pulsars Vela, Crab, and PSR0525 + 21, following sudden jumps or glitches in these quantities. Theoretical aspects of neutron and proton superfluids in neutron stars and core neutron communication, glitches and post-glitch relaxation, neutron star coupling, and vortex creep theory are discussed. The effects of the superfluid interior in the accreting neutron star X-ray sources are also considered.

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