SuperGZK neutrinos: testing physics beyond the Standard Model

Details SuperGZK neutrinos: testing physics beyond the Standard Model SuperGZK neutrinos: testing physics beyond the Standard Model

2003-03-12

arxiv.org/abs/hep-ph/0303091v1

Physics

High Energy Physics

High Energy Physics - Phenomenology

JD talk at XXI Texas Symposium (Florence)

Scientific paper

The sources and fluxes of superGZK neutrinos, $E>10^{20}$ eV, are discussed.
The most promising sources are reionization bright phase, topological defects,
superheavy dark matter and mirror matter. The energy of neutrinos can be above
the GUT scale ($\sim 10^{16}$ GeV). The predicted fluxes are observable by
future space detectors EUSO and OWL.

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