High energy cosmic ray signature of quark nuggets

Details High energy cosmic ray signature of quark nuggets High energy cosmic ray signature of quark nuggets

Aug 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985icrc....8..290a&link_type=abstract

In NASA. Goddard Space Flight Center 19th Intern. Cosmic Ray Conf., Vol. 8 p 290-293 (SEE N85-36066 24-93)

Astronomy and Astrophysics

Astronomy

Black Holes (Astronomy), Charged Particles, Cosmic Ray Showers, Galactic Structure, High Energy Interactions, Magnetic Dipoles, Magnetic Stars, Neutron Stars, Quarks, Relativistic Particles, Electrostatic Charge, Galactic Cosmic Rays, Magnetic Fields

Scientific paper

It has been recently proposed that dark matter in the Universe might consist of nuggets of quarks which populate the nuclear desert between nucleons and neutron star matter. It is further suggested that the Centauro events which could be the signature of particles with atomic mass A approx. 100 and energy E approx. 10 to 15th power eV might also be related to debris produced in the encounter of two neutron stars. A further consequence of the former proposal is examined, and it is shown that the production of relativistic quark nuggets is accompanied by a substantial flux of potentially observable high energy neutrinos.

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