A study of the e+e- --> 3γ process in strong magnetic fields

Details A study of the e+e- --> 3γ process in strong magnetic fields A study of the e+e- --> 3γ process in strong magnetic fields

Jul 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994cha%26a..18..241p&link_type=abstract

Chinese Astronomy and Astrophysics, Volume 18, Issue 3, p. 241-247.

Astronomy and Astrophysics

Astrophysics

Neutron Star, Stellar Magnetic Field, Γ-Ray Burst

Scientific paper

In this paper we study the e+e- --> 3γ process in strong magnetic fields on the basis of quantum electrodynamics. Formulas for the cross section and annihilation rate are obtained in the general case. A numerical calculation for the case of rest annihilation shows that the e+e- --> 3γ process makes a nonnegligible contribution to low-energy emission in not-too-high magnetic fields.

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