Probing Early Universe Physics with Cosmic, Gamma-Ray, and Neutrino Astrophysics

Details Probing Early Universe Physics with Cosmic, Gamma-Ray, and Neutrino Astrophysics Probing Early Universe Physics with Cosmic, Gamma-Ray, and Neutrino Astrophysics

Dec 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998tx19.confe.644s&link_type=abstract

Abstracts of the 19th Texas Symposium on Relativistic Astrophysics and Cosmology, held in Paris, France, Dec. 14-18, 1998. Eds.:

Astronomy and Astrophysics

Astrophysics

Scientific paper

New particle physics beyond the standard model is expected to play an important role in the early universe. Some of the possible resulting processes such as decaying topological defects or massive, long-lived dark matter particles, can contribute to the cosmic and gamma-radiation observed today. This data thus constrains and probes early universe physics. In addition, such processes could give rise to a relic ultra-high energy neutrino flux that could be detected with future neutrino telescopes. We discuss recent results and future prospects in this field.

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