The Spectrum of Secondary Antiprotons

Details The Spectrum of Secondary Antiprotons The Spectrum of Secondary Antiprotons

Aug 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001icrc....5.1873s&link_type=abstract

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

Physics

2

Scientific paper

The cosmic-ray antiproton spectrum may be an important tool for understanding and constraining the nature of dark matter and baryon-symmetric cosmological models. Its understanding requires a good theoretical modeling of antiprotons produced as secondary particles in the interactions of high-energy protons and nuclei with interstellar gas. The production rate of antiprotons in cosmic-ray interactions depends on physical and astrophysical parameters whose values have recently been revised and refined. In this paper we describe the wind-diffusion model of antiprotons and discuss uncertainties in the flux calculation.

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