Published January 1, 2018 | Version v1
Journal article

Detection of MeV scale neutrinos and the solar energy paradigm

Creators

  • 1. Canfranc Underground Laboratory, Paseo de los Ayerbe, s/n, E-22880 Canfranc Estación (Spain)

Description

The fundamental solar energy paradigm establishes that the energy in the Sun is due to a series of nuclear reactions which turn hydrogen into helium. In particular, for the Sun the fundamental reaction corresponds to p + pd + e + + υ e + 0.42 MeV. This is a very slow process which drives the evolution of the Sun over a timescale of 109 years. Electron neutrinos produced in the core interact only weakly and travel almost undisturbed from the core to the surface. They are a unique probe to explore the interior of stars. Observations of solar neutrinos are discussed in the paper. The solar energy paradigm proposed in 1938 by H. Bethe has been measured in realtime by Borexino at 10% level in 2014. This observation allows to probe the solar stability over a 105 years timescale. At present, solar neutrinos offer the opportunity to understand the new Solar Abundance Problem, that is our lack of knowledge of the chemical composition of the Sun. Therefore, improving solar neutrino measurements is of great interest for astrophysics. At the same time, a better determination of some astrophysical factors will reduce uncertainties on predictions to better identify a possible inadequate assumption in the solar model. (paper)

Availability note (English)

Available from http://dx.doi.org/10.1088/1742-6596/940/1/012023

Additional details

Publishing Information

Journal Title
Journal of Physics. Conference Series (Online)
Journal Volume
940
Journal Issue
1
Journal Page Range
[6 p.]
ISSN
1742-6596

Conference

Title
7. Nuclear Physics in Astrophysics Conference
Dates
18-22 May 2015
Place
York (United Kingdom)