ecCNO Solar Neutrinos: A Challenge for Gigantic Ultra-Pure Liquid Scintillator Detectors

Abstract

Neutrinos produced in the Sun by electron capture reactions on ${}^{13}\mathrm{N}$, ${}^{15}\mathrm{O}$ and ${}^{17}\mathrm{F}$, to which we refer as ecCNO neutrinos, are not usually considered in solar neutrino analysis since the expected fluxes are extremely low. The experimental determination of this sub-dominant component of the solar neutrino flux is very difficult but could be rewarding since it provides a determination of the metallic content of the solar core and, moreover, probes the solar neutrino survival probability in the transition region at $E_{\nu }\sim 2.5\mathrm{MeV}$. In this letter, we suggest that this difficult measure could be at reach for future gigantic ultra-pure liquid scintillator detectors, such as LENA.

11 pages

References in corpus (3)

• Helioseismology and Solar Abundances
• Detecting the Upturn of the Solar ${}^8$B Neutrino Spectrum with LENA
• The Physics Potential of the LENA Detector

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