Relaxation times in superfluid cores of neutron stars

Details Relaxation times in superfluid cores of neutron stars Relaxation times in superfluid cores of neutron stars

Jan 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985afz....22..137s&link_type=abstract

(Astrofizika, vol. 22, Jan.-Feb. 1985, p. 137-144) Astrophysics (ISSN 0571-7132), vol. 21, no. 1, July 1985, p. 84-88. Translati

Astronomy and Astrophysics

Astrophysics

6

Neutron Stars, Relaxation Time, Stellar Cores, Stellar Models, Stellar Rotation, Superfluidity, Electron Scattering, Proton Density (Concentration), Pulsars, Relativistic Electron Beams, Stellar Magnetic Fields, Strong Interactions (Field Theory), Vortex Filaments

Scientific paper

The velocity relaxation times of normal electrons on the proton flux
lines occurring on account of the drag effect in the "npe"-phase of a
neutron star are considered. It is shown that the "npe"-phase is rigidly
connected with the star crust.

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