Statistics – Computation
Scientific paper
Nov 1984
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984afz....20..547s&link_type=abstract
(Astrofizika, vol. 20, Nov.-Dec. 1984, p. 547-561) Astrophysics (ISSN 0571-7132), vol. 20, no. 6, May 1985, p. 656-664. Translat
Statistics
Computation
Baryons, Magnetic Moments, Neutron Stars, Rotating Fluids, Stellar Magnetic Fields, Angular Velocity, Computational Astrophysics, Neutrons, Superfluidity, Vortex Filaments
Scientific paper
The generation of a magnetic field in a spherical neutron star of a real baryon gas is investigated theoretically, applying the results obtained in the London approximation by Sedrakian and Shakhabasian (1972 and 1980), Sedrakian (1982), and Sedrakian et al. (1983) for an infinite cylinder of constant matter denstiy. In the rotating npe superfluid solution, the formation of rectilinear neutron vortices parallel to the rotation axis by entrainment of protons by neutrons, the induction of an inhomogeneous magnetic field, and the appearance of an entrained-proton vortex lattice of entrained protons with a dipole magnetic field are predicted. The magnetic moment is calculated numerically for neutron stars of mass 0.149-0.688 solar mass, radius 10.0-11.5 km, and density 184-601 Tg/cu cm and found to vary from (2 to 927) x 10 to the 27th G/cu cm.
Movsisian A. G.
Sedrakian David M.
Shakhabasian K. M.
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