Pulsar Contribution to High Energy Cosmic Rays

Details Pulsar Contribution to High Energy Cosmic Rays Pulsar Contribution to High Energy Cosmic Rays

Aug 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001icrc....6.2092g&link_type=abstract

Proceedings of the 27th International Cosmic Ray Conference. 07-15 August, 2001. Hamburg, Germany. Under the auspices of the Int

Physics

3

Scientific paper

We show that assuming a simple CR acceleration scenario, where all the pulsar rotational energy is transformed into CR particles of the highest available energy at a given moment, one obtains particle fluxes of the order of the observed ones. The slope of CR energy spectrum for E>1016 eV would be determined by a powerlaw distribution of their initial periods and the spectrum flattening - by the decay of the pulsar magnetic field.

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