Studying low-energy astrophysical neutrinos with neutrino nucleus cross-section calculations and beta beam neutrino spectra

Details Studying low-energy astrophysical neutrinos with neutrino nucleus cross-section calculations and beta beam neutrino spectra Studying low-energy astrophysical neutrinos with neutrino nucleus cross-section calculations and beta beam neutrino spectra

Apr 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011prpnp..66..424t&link_type=abstract

Progress in Particle and Nuclear Physics, Volume 66, Issue 2, p. 424-429.

Physics

Nuclear Physics

2

Scientific paper

We first calculate total neutrino-nucleus cross-sections for the reactions 66Zn)66Zn and 130Te)130Te within the context of the quasi-particle random phase approximation. The isotopes 66ZnTe are contents of the COBRA double beta decay detector at Gran Sasso. We then use synthetic low-energy beta-beam antineutrino spectra, originating from boosted β- radioactive 6He ions for the interpretation of various SN-neutrino signals.

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