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

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.

15 pages, 7 figures, Invited talk at the XXIII International Conference on Neutrino Physics and Astrophysics, Christchurch, New Zealand, May 25 - 31, 2008

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Cited by in corpus (3)

• Updated fit to three neutrino mixing: status of leptonic CP violation
• Common Origin of Soft mu-tau and CP Breaking in Neutrino Seesaw and the Origin of Matter
• Neutrino mass observables and non-Hermitian version of Type-I seesaw model