On the requirements for acceleration mechanisms to produce flattened heavy particle cosmic ray energy spectra

Details On the requirements for acceleration mechanisms to produce flattened heavy particle cosmic ray energy spectra On the requirements for acceleration mechanisms to produce flattened heavy particle cosmic ray energy spectra

Apr 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975ap%26ss..33..459w&link_type=abstract

Astrophysics and Space Science, vol. 33, Apr. 1975, p. 459-463.

Physics

Cosmic Rays, Energy Spectra, Heavy Nuclei, Pulsars, Radiation Spectra, Acceleration (Physics), Astronomical Models, Energy Dissipation, Gravitational Waves, Stellar Evolution, Supernovae

Scientific paper

The recently observed flattening of the energy spectra of high Z
particles is investigated in terms of the limits it places on
acceleration mechanisms. The possibility of a new mechanism is suggested

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