Neutrino-2008: Where are we? Where are we going?

TL;DR

This paper reviews the current understanding of neutrino physics, discusses future experimental and theoretical directions, and highlights the potential for new discoveries in neutrino astrophysics, collider physics, and cosmology.

Contribution

It provides a comprehensive overview of the standard neutrino scenario, recent developments, and outlines future research goals and technological advancements in neutrino studies.

Findings

Confirmation of neutrino oscillations and mass

Potential for new physics beyond the standard model

Development of advanced neutrino detection techniques

Abstract

Our present knowledge of neutrinos can be summarized in terms of the "standard neutrino scenario". Phenomenology of this scenario as well as attempts to uncover physics behind neutrino mass and mixing are described. Goals of future studies include complete reconstruction of the neutrino mass and flavor spectrum, further test of the standard scenario and search for new physics beyond it. Developments of new experimental techniques may lead to construction of new neutrino detectors from table-top to multi-Megaton scales which will open new horizons in the field. With detection of neutrino bursts from the Galactic supernova and high energy cosmic neutrinos neutrino astrophysics will enter qualitatively new phase. Neutrinos and LHC (and future colliders), neutrino astronomy, neutrino structure of the Universe, and probably, neutrino technologies will be among leading topics of research.