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- W3014010781 abstract "Tau Air-showers are the best trace of rarest Ultra High Energy neutrinos UHE $nu_{tau}$, $barnu_{tau}$ and $bar{nu}_e$ at PeV and higher energy. $tau$ Air-showers may generate billion times amplified signals by their secondaries . Horizontal amplified $tau$ air-showers by $nu_{tau} N$ and UHE $barnu_{e} e$ at PeV emerging from mountain chain might be the most power-full imprint. Upward UHE $nu_{tau} N$ interaction on Earth crust at horizontal edge and from below, their consequent UHE $tau$ air-showers beaming toward high mountains should flash $gamma$,$mu$,X and optical detectors on the top. Upward $tau$ air-shower may hit nearby satellite flashing them by short, hard, diluted $gamma-$burst at the edge of Gamma Ray Observatory BATSE threshold. We identify these events with recent (1994) discovered upward Terrestrial Gamma Flashes (TGF) and we probed their UHE $tau$ - UHE $nu_tau$ origin. From these TGF data approximated UHE $nu_tau$ flux and $Delta m_{nu_mu nu_tau}$ sever lower bound are derived. Partial TGF Galactic signature is also manifest within known 47 TGF events clustered within three degrees from the Galactic plane at ${simeq 2cdot 10^{-3}}$probability. Well known $X-gamma-mathrm{TeV}$ active galactic and extragalactic sources have found probable counterpart in TGF arrival directions. Detection of elusive UHE $nu_tau$ seem finally achieved." @default.
- W3014010781 created "2020-04-03" @default.
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- W3014010781 date "2000-05-22" @default.
- W3014010781 modified "2023-09-27" @default.
- W3014010781 title "Detecting Ultra High Energy Neutrinos by Upward Tau Airshowers and Gamma Flashes" @default.
- W3014010781 hasPublicationYear "2000" @default.
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