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Issue A&A Volume 423, Number 2, August IV 2004 Page(s) 405 - 413 Section Astrophysical processes DOI 10.1051/0004-6361:20047005

A&A 423, 405-413 (2004)
DOI: 10.1051/0004-6361:20047005

Cosmic rays from Galactic pulsars

W. Bednarek and M. Bartosik

Department of Experimental Physics, University of Lódz, ul. Pomorska 149/153, 90-236 Lódz, Poland
    e-mail: bednar@fizwe4.fic.uni.lodz.pl

(Received 5 January 2004 / Accepted 11 May 2004 )

Abstract
We calculate energy spectra and mass composition of cosmic rays accelerated by the galactic population of pulsars during their radio and gamma-ray phase. It is assumed that a significant part of the pulsar rotational energy is lost on acceleration of iron nuclei extracted from the surface of the neutron star. The nuclei are accelerated, at first when passing the outer gap of the inner pulsar magnetosphere and later in the pulsar wind zone, to energies corresponding to 50% of the total potential drop through the polar cap region of the neutron star. We calculate energy spectra of the nuclei injected from the pulsar wind nebulae into the Galaxy including different energy loss processes of nuclei during their propagation in the pulsar magnetosphere and the expanding nebula, their fragmentation in collisions with radiation and matter, adiabatic energy losses, and escape from the nebula. Several models proposed for the distribution of the initial parameters of the galactic pulsar population are considered. It is shown that the best description of the observed cosmic ray spectrum and the mass composition between a few 10¹⁵ eV and a few 10¹⁸ eV is obtained for the model B of Lorimer et al., in which the logs of initial pulsar periods and surface magnetic fields are given by the Gaussian distributions with the average values of   = 2.6 and   = 12.3, respectively. In order to supply the cosmic rays into the Galaxy with the required rate, the product of the efficiency of cosmic ray acceleration by pulsars and their birth rate should be about  10^-2 yr ^-1.

Key words: stars: supernovae: general -- acceleration of paricles -- stars: pulsars: general -- ISM: cosmic rays

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