Magnetic field decay in isolated neutron stars
1992; IOP Publishing; Volume: 395; Linguagem: Inglês
10.1086/171646
ISSN1538-4357
AutoresPeter Goldreich, Andreas Reisenegger,
Tópico(s)Atomic and Subatomic Physics Research
Resumoview Abstract Citations (472) References (27) Co-Reads Similar Papers Volume Content Graphics Metrics Export Citation NASA/ADS Magnetic Field Decay in Isolated Neutron Stars Goldreich, Peter ; Reisenegger, Andreas Abstract Three mechanisms that promote the loss of magnetic flux from an isolated neutron star - Ohmic decay, ambipolar diffusion, and Hall drift - are investigated. Equations of motions are solved for charged particles in the presence of a magnetic field and a fixed background of neutrons, while allowing for the creation and destruction of particles by weak interactions. Although these equations apply to normal neutrons and protons, the present interpretations of their solutions are extended to cover cases of neutron superfluidity and proton superconductivity. The equations are manipulated to prove that, in the presence of a magnetic force, the charged particles cannot be simultaneously in magnetostatic equilibrium and chemical equilibrium with the neutrons. The application of the results to real neutron stars is discussed. Publication: The Astrophysical Journal Pub Date: August 1992 DOI: 10.1086/171646 Bibcode: 1992ApJ...395..250G Keywords: Charged Particles; Magnetic Flux; Magnetic Stars; Neutron Stars; Stellar Magnetic Fields; Decay; Early Stars; Pulsars; X Ray Binaries; Astrophysics; STARS: MAGNETIC FIELDS; STARS: NEUTRON full text sources ADS |
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