Conditions for stimulated-annihilation in a degenerate electron-positron fluid at the surface of pulsars

Details Conditions for stimulated-annihilation in a degenerate electron-positron fluid at the surface of pulsars Conditions for stimulated-annihilation in a degenerate electron-positron fluid at the surface of pulsars

Jul 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983aipc..101..421v&link_type=abstract

IN: Positron-electron pairs in astrophysics; Proceedings of the Workshop, Greenbelt, MD, January 6-8, 1983 (A85-31276 13-90). Ne

Astronomy and Astrophysics

Astrophysics

1

Annihilation Reactions, Crab Nebula, Degenerate Matter, Gamma Ray Spectra, Pulsars, Stellar Magnetic Fields, Astrophysics, Electrons, Line Spectra, Photons, Positrons, Steady State, Stimulated Emission

Scientific paper

Electrons and positrons in the large magnetic fields at the surface of
pulsars condense into rod shaped droplets. The conditions for stimulated
annihilation in such droplets are examined. The motivation for this
investigation are the observation of Leventhal et al. (1977) of very
narrow gamma-ray lines emanating from the Crab Nebula.

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