Neutrino Mass: Where Do We Stand, and Where Are We Going?
Boris Kayser

TL;DR
This paper reviews current evidence for neutrino mass from atmospheric, solar, and LSND experiments, discusses proposed mass scenarios, and outlines future tests needed to confirm and understand neutrino properties.
Contribution
It provides a comprehensive overview of neutrino mass hints and proposes future experimental directions to clarify neutrino mass mechanisms.
Findings
Strong evidence of neutrino mass from atmospheric neutrinos
Promising hints from solar neutrino observations
Unconfirmed LSND neutrino oscillation hint
Abstract
We discuss the three major hints of neutrino mass: the strong evidence of mass from the behavior of atmospheric neutrinos, the very promising further hint from the behavior of solar neutrinos, and the so-far unconfirmed hint from the LSND experiment. Then, we describe two illustrative neutrino-mass scenarios suggested by the observed hints. We identify the needed future tests of both the present hints and the neutrino-mass scenarios.
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Taxonomy
TopicsNeutrino Physics Research · Astrophysics and Cosmic Phenomena · Dark Matter and Cosmic Phenomena
