1 code implementation • 4 Apr 2016 • David G. Cerdeno, Malcolm Fairbairn, Thomas Jubb, Pedro A. N. Machado, Aaron C. Vincent, Celine Boehm
In this article, we compute the projected nuclear and electron recoil rates expected in several dark matter direct detection experiments due to solar neutrinos, and use these estimates to quantify errors on future measurements of the neutrino fluxes, weak mixing angle and solar observables, as well as to constrain new physics in the neutrino sector.
High Energy Physics - Phenomenology
