8B and hep solar neutrino detection by terrestrial experiments


Published: Nov 23, 2019
G. I. Karathanou
V. S. Tsikoudi
T. S. Kosmas
Abstract

Solar neutrino spectra of 8B and hep neutrinos produced by pp-chain reactions are analysed for various nuclear detectors in current terrestrial experiments. The well known folding method is applied by employing appropriately simulated solar neutrino distributions and using recently calculated total cross section of neutrino- nucleus processes. We focus on the nuclear target of current experiments like MOON and ICARUS as well to other promising nuclear isotopes.

Article Details
  • Section
  • Oral contributions
References
E. Kolbe and T.S. Kosmas, Springer Trac. Mod. Phys. 163, 199 225 (2000).
A. Drukieer and L. Stodolsky, Phys. Rev. D 30, 2295, (1984).
J. Bahcall, Neutino Astrophysics (Cambridge University, Cambridge) (1989).
W.C. Haxton, P.D. Parker and C.E. Rolfs, nucl-th/0501020v1, (2005).
T.S. Kosmas, Nucl. Phys. A 683, 443 (2001).
G.I. Karathanou, V. Tsikoudi, Th. Liolios and T.S. Kosmas, 17th Symposium of The Hellenic Nuclear Physics Society, Ioannina, May, 2008
G.I. Karathanou, V. Tsikoudi, Th. Liolios and T.S. Kosmas, in preparation.
J.D. Vergados and H. Ejiri, 2008, hep-ph/0805.2583v2