Parity nonconservation and the origin of cosmic magnetic fields

Details Parity nonconservation and the origin of cosmic magnetic fields Parity nonconservation and the origin of cosmic magnetic fields

Mar 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982apj...254...77v&link_type=abstract

Astrophysical Journal, Part 1, vol. 254, Mar. 1, 1982, p. 77-81. Research supported by the Natural Sciences and Engineering Res

Astronomy and Astrophysics

Astronomy

14

Black Holes (Astronomy), Field Strength, Interstellar Magnetic Fields, Parity, Asymmetry, Electric Current, Electromagnetic Fields, Particle Emission, Proton Flux Density, Weak Energy Interactions

Scientific paper

Three mechanisms of cosmic magnetic field generation are discussed: (1) asymmetric decay of particles emitted by rotating black holes; (2) asymmetric proton emission by black holes due to weak radiative corrections, and (3) equilibrium parity-violating currents. It is shown that all three mechanisms can produce a seed field sufficiently strong to account for the present galactic fields.

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