Paramagnetic effects in a superconducting neutron star

Details Paramagnetic effects in a superconducting neutron star Paramagnetic effects in a superconducting neutron star

Nov 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986afz....25..533s&link_type=abstract

(Astrofizika, vol. 25, Nov.-Dec. 1986, p. 533-543) Astrophysics (ISSN 0571-7132), vol. 25, no. 3, May 1987, p. 665-671. Translat

Physics

Condensed Matter

Superconductivity

3

Neutron Stars, Paramagnetism, Superconductivity, Equations Of State, Particle Spin, Protons

Scientific paper

The effect of Pauli spin paramagnetism on the mixed state in the "npe"-phase of a neutron star is considered. The drag of superfluid protons by rotating superfluid neutrons is also taken into account. It has been shown that the Fulde-Ferrell state cannot exist in a neutron star with hard equation of state. The value of second-order transition field Hc2 decreases. The characteristics of a type II proton superconductor are calculated as functions of density.

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