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Damping signatures in future neutrino oscillation experiments

Mattias Blennow1, Tommy Ohlsson1 and Walter Winter2

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We discuss the phenomenology of damping signatures in the neutrino oscillation probabilities, where either the oscillating terms or the probabilities can be damped. This approach is a possibility for tests of damping effects in future neutrino oscillation experiments, where we mainly focus on reactor and long-baseline experiments. We extensively motivate different damping signatures due to small corrections by neutrino decoherence, neutrino decay, oscillations into sterile neutrinos, or other mechanisms, and classify these signatures according to their energy (spectral) dependencies. We demonstrate, at the example of short baseline reactor experiments, that damping can severely alter the interpretation of results, e.g., it could fake a value of sin2θ13 smaller than the one provided by Nature. In addition, we demonstrate how a neutrino factory could constrain different damping models with emphasis on how these different models could be distinguished, i.e., how easily the actual type of effect could be identified. We find that the damping models cluster in different categories, which can be much better distinguished from each other than models within the same cluster.

Keywords

Neutrino Physics

Solar and Atmospheric Neutrinos

 

E-print Number: hep-ph/0502147

Cited: by |

Refers: to

PACS

14.60.Lm Ordinary neutrinos (nue, numu, nutau)

96.60.Jw Solar interior

96.50.sb Composition, energy spectra and interactions

13.35.-r Decays of leptons

96.60.Vg Particle emission, solar wind

96.50.Vg Energetic particles

Subjects

Particle physics and field theory

Astrophysics and astroparticles

Dates

Issue 06 (June 2005)

Received 25 February 2005, accepted for publication 23 May 2005

Published 17 June 2005



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