Electrons and positrons from expanding supernova envelopes in dense clouds

Details Electrons and positrons from expanding supernova envelopes in dense clouds Electrons and positrons from expanding supernova envelopes in dense clouds

Aug 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985icrc....2..390s&link_type=abstract

In NASA. Goddard Space Flight Center 19th Intern. Cosmic Ray Conf., Vol. 2 p 390-393 (SEE N85-34006 22-93)

Computer Science

Clouds, Cosmic Rays, Electrons, Positrons, Stellar Envelopes, Stellar Radiation, Supernovae, Differential Equations, Energy Spectra, Nucleons

Scientific paper

If antiprotons in cosmic rays are produced as secondary particles in
sources, it is expected that positrons are also created by the same
process. The interstellar spectra of positrons and electrons are
calculated by taking into account such sources. Spectra are then
compared with observations.

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