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Cosmic rays from PeV to ZeV, stellar evolution, supernova physics and gamma ray bursts

2003

Author(s): Biermann, PL (Biermann, PL); Moiseenko, S (Moiseenko, S); Ter-Antonyan, S (Ter-Antonyan, S); Vasile, A (Vasile, A)


Edited by: Sanchez NG; Parijskij YN


Source: EARLY UNIVERSE AND THE COSMIC MICROWAVE BACKGROUND: THEORY AND OBSERVATIONS  Book Series: NATO Science Series II-Mathematics Physics and Chemistry  Volume: 130  Pages: 489-516  Published Date: 2003   

Abstract: The recent success of a proposal from some time ago to explain the spectrum of cosmic rays allows some strong conclusions to be made on the physics of supernovae: In the context of this specific proposal to explain the origin of cosmic rays, the mechanism for exploding supernovae of high mass has to be the one proposed by Bisnovatyi-Kogan more than 30 years ago, which was then based on a broader suggestion by Kardashev: A combination of the effects of rotation and magnetic fields explodes the star. Interestingly, this step then leads inevitably to some further suggestions, useful perhaps for the study of gamma ray bursts and the search of a bright standard candle in cosmology.

Accession Number: WOS:000221382600022

Conference Title: Conference of the NATO-Advanced-Study-Institute on the Early Universe and the Cosmic Microwave Background

Conference Date: SEP 07-20, 2002

Conference Location: Palermo, ITALY

Conference Sponsors: NATO Adv Study Inst