Astronomy and Astrophysics – Astrophysics
Scientific paper
Apr 1994
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994ap%26ss.214...89p&link_type=abstract
Astrophysics and Space Science, Vol. 214, No. 1-2, Proceedings of the second United Nations/European Space Agency Workshop, Bogo
Astronomy and Astrophysics
Astrophysics
Annihilation Reactions, Eigenvectors, Quantum Electrodynamics, Stellar Magnetic Fields, Electron-Positron Pairs, Magnetic Effects, Neutron Stars, Positron Annihilation, Red Shift
Scientific paper
We report specifically on a quantum electrodynamic feature of the one-photon-pair annihilation. Most of the calculation related with this process (not excluding other ones) have been carried out usually utilizing the wave functions obtained from the Dirac equation in the Landau gauge Aa = (0, Bx, 0), where B is oriented along the z-axis (Johnson and Lippman, 1949). Although, the eigenstates of the Dirac Hamiltonian as it was introduced by Johnson and Lippman, do not consider the coupling to the radiation field and consequently they reflect only for pz = 0 the same linear combination of the two degenerate polarization states. We report the transition rate function for the one-photon-pair annihilation in a strong magnetic field by using the Sokolov and Ternov eigenstate +/- as far as pz = 0 and N greater than 0 is concerned. The difference between the expression for the transition rate by using the Sokolov and Ternov eigenstates and the one calculated by Wunner et al., 1986, is just the function Is, s' which corresponds to the degeneracy of the orbit center of the electrons characterized by the quantum numbers s and s'.
Bonatti Javier
Páez Jorge
Semionova Luidmila
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