This project is dedicated but not limited to the study and minimization of uncertainties in the extracting the neutrino
mixing parameters and squared-mass splittings by analyzing data from neutrino oscillation experiments involving atmospheric,
solar, astrophysical, accelerator and reactor (anti) neutrinos.
Although the problem itself is by no means new, we intend to improve the accuracy of the global neutrino oscillation analysis
by developing phenomenology of (anti)neutrino interactions with matter,
by adjusting the (anti)neutrino-nucleus cross sections (and related observables) using the most extensive and complete datasets,
by improving the classical and quantum neutrino transport theory,
by developing the neutrino oscillation theory (mainly within a field-theoretical approach).
On this page, we will post current and upcoming results and related issues that reflect our team's progress.
Astroparticle Physics European Coordination 
