Annihilation Lines 255.5 and 511 keV in the Radiation Spectrum from the Pulsar Polar Cap

Details Annihilation Lines 255.5 and 511 keV in the Radiation Spectrum from the Pulsar Polar Cap Annihilation Lines 255.5 and 511 keV in the Radiation Spectrum from the Pulsar Polar Cap

Aug 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aipc.1269..451k&link_type=abstract

THE 10TH INTERNATIONAL SYMPOSIUM ON ORIGIN OF MATTER AND EVOLUTION OF GALAXIES: OMEG-2010. AIP Conference Proceedings, Volume 1

Physics

1

Pulsars, Gamma-Rays, Neutron Stars, Ionisation, Pulsars, Gamma-Ray, Neutron Stars, Electronic Excitation And Ionization Of Molecules, Intermediate Molecular States

Scientific paper

We consider the formation of lines 255.5 keV and 511 keV due to
annihilation of fast positrons from the pulsar vacuum gap with slow
electrons of the neutron star surface. The weak line 255.5 keV can be
detected by observing the opposite (to the positron stream) radiation in
the laboratory experiment.

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