Ultrahigh-energy particle flux from cosmic strings

Details Ultrahigh-energy particle flux from cosmic strings Ultrahigh-energy particle flux from cosmic strings

Apr 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990stin...9022525b&link_type=abstract

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Computer Science

Cosmic Rays, Cosmology, Gravitational Collapse, Protons, String Theory, Coronal Loops, Flux (Rate), Universe

Scientific paper

The expected flux is estimated of ultrahigh energy (greater than 1018 eV) protons in the present epoch due to a process which involves collapse or multiple self-intersections of a special class of closed cosmic string loops in the universe. This flux is compared with the observed flux of ultrahigh energy cosmic rays, and the implications are discussed.

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