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Autori principali: Hellmann, Dominik, Krieg, Sara, Päs, Heinrich, Tabet, Mustafa
Natura: Preprint
Pubblicazione: 2024
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Accesso online:https://arxiv.org/abs/2405.05000
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author Hellmann, Dominik
Krieg, Sara
Päs, Heinrich
Tabet, Mustafa
author_facet Hellmann, Dominik
Krieg, Sara
Päs, Heinrich
Tabet, Mustafa
contents Gravitational waves (GWs) can alter the neutrino propagation distance and thus affect neutrino oscillations. This can result in a complete disappearance of the oscillatory behavior that competes with other sources of neutrino decoherence. We develop a set of criteria that determines under which conditions neutrino oscillations are sensitive to this effect. We find that current or near future neutrino oscillation experiments are not sufficiently sensitive to coherent GW signals but may probe the stochastic gravitational wave background if the energy resolution improves drastically by several orders of magnitude.
format Preprint
id arxiv_https___arxiv_org_abs_2405_05000
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle Neutrino Oscillations as a Gravitational Wave Detector?
Hellmann, Dominik
Krieg, Sara
Päs, Heinrich
Tabet, Mustafa
High Energy Physics - Phenomenology
Gravitational waves (GWs) can alter the neutrino propagation distance and thus affect neutrino oscillations. This can result in a complete disappearance of the oscillatory behavior that competes with other sources of neutrino decoherence. We develop a set of criteria that determines under which conditions neutrino oscillations are sensitive to this effect. We find that current or near future neutrino oscillation experiments are not sufficiently sensitive to coherent GW signals but may probe the stochastic gravitational wave background if the energy resolution improves drastically by several orders of magnitude.
title Neutrino Oscillations as a Gravitational Wave Detector?
topic High Energy Physics - Phenomenology
url https://arxiv.org/abs/2405.05000