Antiproton generation in giant molecular clouds

Details Antiproton generation in giant molecular clouds Antiproton generation in giant molecular clouds

May 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988pazh...14..417d&link_type=abstract

Pis'ma v Astronomicheskii Zhurnal (ISSN 0320-0108), vol. 14, May 1988, p. 417-424. In Russian.

Astronomy and Astrophysics

Astronomy

1

Antiprotons, Cosmic Rays, Molecular Clouds, Disk Galaxies, Galactic Structure, Milky Way Galaxy

Scientific paper

The antiproton spectrum for cosmic rays near the earth is calculated using a model in which antiprotons are ejected by giant molecular clouds situated in the Galactic disk. It is suggested that the charged particles inside the clouds are accelerated via the statistical acceleration mechanism. It is shown that this model can be used to describe the features of the observed antiproton spectrum in the 0.4-15 GeV energy range.

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