γ-positronium in strong magnetic fields

Physics

Scientific paper

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Scientific paper

The probabilities of positronium-photon and photon-positronium transitions in a magnetic field α2H0 << H  H0 have been calculated (H0=m20c3/eh=4.4×1013 G, α=e2/hc=1/137). We consider the propagation of a photon with an energy exceeding the positronium energy in curved lines of force in the magnetosphere of a pulsar. The possibility of γ --> γ1 + γ2 decay through the intermediate positronium state is discussed.

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