2001/05/14 by Sandip Pakvasa, Pakvasa, Sandip
Physics and Astronomy · #Astrophysics (astro-ph) #Astrophysics and Cosmic Phenomena #FOS: Physical sciences #High Energy Physics - Experiment (hep-ex) #High Energy Physics - Phenomenology (hep-ph) #Neutrino Physics Research #astro-ph #hep-ex #hep-ph
paper · pdf · doi:10.48550/arxiv.hep-ph/0105127
10PAGES; Invited talk presented at Neutrino Telescopes Workshop, Venice, March 6-9, 2001; to be published in the proceedings
arxiv created 2001/05/14 · openalex publication_date 2001/05/14 · arxiv updated 2009/11/30 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28
We imagine that large neutrino telescopes will be built and that distant neutrino sources of high energies and fluxes exist. Some possible, if difficult, uses to which they might be put are described; including (i) detecting neutrino mass-mixing possibly upto delta m2 of 10-16eV2; (ii) measuring neutrino cross-sections at PeV energies; (iii) detecting relic neutrinos; (iv) doing cosmology with neutrinos and (v) SETI with neutrinos.