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arXiv · 1809.02004

Solar neutrino flare, megaton neutrino detectors and human space journey

Daniele Fargion·Pietro Oliva·P. G. De Sanctis Lucentini·Silvia Pietroni·Fabio La Monaca·Paolo Paggi·Emanuele Habib·Maxim Yu. Khlopov
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Abstract

The largest solar flare have been recorded in gamma flash and hard spectra up to tens GeV energy. The present building and upgrade of Hyper- Kamiokande (HK) in Japan and Korea, (as well as Deep Core, PINGU) Megatons neutrino detectors do offer a novel way to detectable trace of solar flares: their sudden anti-neutrino (or neutrino) imprint made by proton scattering and pion decays via Delta resonance production on solar corona foot-point. These signals might be observable at largest flare by HK via soft spectra up to tens-hundred MeV energy and by IceCube-PINGU at higher, GeVs energies. We show the expected rate of signals for the most powerful solar flare occurred in recent decades extrapolated for future Megaton detectors. The neutrino solar flare detection with its prompt alarm system may alert astronauts on space journey allowing them to hide themselves into inner rocket container surrounded by fuel or water supply. These container walls are able to defend astronauts from the main lethal (the dominant soft component) radiation wind due to such largest solar flares.

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Daniele Fargion, Pietro Oliva, P. G. De Sanctis Lucentini, Silvia Pietroni, Fabio La Monaca, Paolo Paggi, Emanuele Habib, Maxim Yu. Khlopov. 2018-11-18. Solar neutrino flare, megaton neutrino detectors and human space journey. https://doi.org/10.1142/9789811204296_0025

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