Cosmic Thermal Neutrino Background: Can it be Detected?

Details Cosmic Thermal Neutrino Background: Can it be Detected? Cosmic Thermal Neutrino Background: Can it be Detected?

Dec 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997japa...18..263b&link_type=abstract

Journal of Astrophysics and Astronomy, Vol. 18, p.263

Mathematics

Logic

Cosmic Neutrino Background, Cosmic Rays, Massive Neutrino, Topological Defects.

Scientific paper

The detection of the Cosmic Thermal Neutrino Background (CTNB) would provide the "cleanest" evidence for the hot big bang model of the early Universe. I discuss some recent thoughts on the possibility of detecting the CTNB (especially if neutrinos have a small mass of ~ few eV) by looking for certain CTNB-induced features in the extremely high energy (E >~ 10(sup 20) eV) cosmic neutrino spectrum that may become measurable in the future by some of the large-area extensive air-shower detectors being built for detecting extremely high energy cosmic rays.

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