Pair annihilation in superstrong magnetic fields

Details Pair annihilation in superstrong magnetic fields Pair annihilation in superstrong magnetic fields

May 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980apj...238..296d&link_type=abstract

Astrophysical Journal, Part 1, vol. 238, May 15, 1980, p. 296-310.

Astronomy and Astrophysics

Astrophysics

42

Neutron Stars, Particle Interactions, Positron Annihilation, Stellar Magnetic Fields, Astrodynamics, Field Strength, Magnetic Effects, Pair Production, Pulsars

Scientific paper

The kinematical and dynamical aspects of the annihilation processes in superstrong magnetic fields are studied. The feasibility and potential significance of detecting from magnetic neutron stars are discussed. The discussion proceeds from the derivation of the fully relativistic differential cross sections and annihilation rates for both one- and two-photon emission from a ground-state gas of electrons and positrons in a static, uniform magnetic field.

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