In this module we show how neutrinos can come from diferent sources: Big Bang, sun, atmosphere, accelerators, supernovae, cosmos, ... We explain basic characteristics of these diferent neutrinos and finish with another practical exercise on the principle of detection for Water Cherenkov Detectors.

In this module we present the basic theory in fundamental physics, the Standard Model and we see how neutrinos are related with each of the fundamental forces: electromagnetism, strong force and weak force. We also introduce the concepts of helicity and chirality and discuss the relation with neutrinos.

In this module we discuss the important concept of neutrino oscillations. In order to this we introduce eigenstates, the PMNS matrix and the concept of oscillation probability. We apply all this to the practical case of DUNE.

In this module we see basic notions for neutrino detection. We present some examples of near detectors in the Kamioka projects and the case of NOvA and DUNE. We finish with the important concept of cross-section and its application to the detection of solar neutrinos with Super-Kamiokande.

In this module we discuss future ares for neutrino field: matter-antimatter asymmetry, prospects for neutrino mass determination, importance of neutrino research in the search for Physics Beyond the Standard Model, relevance of neutrinos in Astrophysics and Cosmology, and some basic notions about Applications in Science and Technology.