Speaker
Dr
Mariam Tórtola
(Universität Hamburg)
Description
The presence of neutrino oscillations in the solar neutrino flux is
nowadays a fact supported by all the existing solar neutrino
experiments and unambiguously confirmed by the reactor experiment
KamLAND. In this talk we will review the current status of the solar
neutrino parameter determination after the latest results from the
Sudbury and Borexino solar experiments. We will also discuss the robustness
of the oscillation interpretation of solar neutrino data with respect
to the presence of non-standard neutrino properties or non-standard
physics in the Sun.
Primary author
Dr
Mariam Tórtola
(Universität Hamburg)
