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Cited by 454

The DOI matches its Crossref record; 3 of the 3 references it cites were found in a registry or an index.

Detecting ντ oscillations at PeV energies

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Learned, John G, Pakvasa, Sandip·1995·Astroparticle Physics

Abstract

It is suggested that a large deep underocean neutrino detector, given the presence of significant numbers of neutrinos in the PeV range as predicted by various models of Active Galactic Nuclei, can make unique measurements of the properties of neutrinos. It will be possible to observe the existence of the nu_tau, measure its mixing with other flavors, in fact test the mixing pattern for all three flavors based upon the mixing parameters suggested by the atmospheric and solar neutrino data, and measure the nu_tau cross section. The key signature is the charged current nu_tau interaction, which produces a double cascade, one at either end of a minimum ionizing track. At a few PeV these cascades would be separated by roughly 100 m, and thus be easily resolvable in DUMAND and similar detectors. Future applications are precise neutrino astronomy and earth tomography.

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Metadata

Authors
Learned, J. G., & Pakvasa, S.
Venue
Astroparticle Physics
Publisher
Elsevier BV
Published
1995-05
Volume
3
Issue
3
Pages
267-274
ISSN
0927-6505 (ISSN-L)
OpenAlex
W1515826804
Cited by
454
References
3
FWCI
4.17
Type
journal article
Language
en
Open access
green

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CoChat. (2026). Citation check: Detecting ντ oscillations at PeV energies. https://app.cochat.ai/papers/10.1016/0927-6505(94)00043-3
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Learned, J. G., & Pakvasa, S. (1995). Detecting ντ oscillations at PeV energies. Astroparticle Physics. https://doi.org/10.1016/0927-6505(94)00043-3

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