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Article . 1994 . Peer-reviewed
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Three-flavor vacuum oscillations of atmospheric and solar neutrinos

descriptionPublicationkeyboard_double_arrow_right Article 01 Jan 1994 English Publisher:American Physical Society (APS)Journal:Physical Review D, volume 49, pages 328-332 (issn: 0556-2821, Copyright policy )
Authors: , Acker; , Balantekin; , Loreti;

doi: 10.1103/physrevd.49.328

pmid: 10016771

Three-flavor vacuum oscillations of atmospheric and solar neutrinos

Abstract

Vacuum oscillations of [nu][sub [mu]] into [nu][sub [tau]] and either matter-enhanced or just-so'' vacuum oscillations of [nu][sub [ital e]] into [nu][sub [mu]] are generally invoked to explain the observed discrepancies in atmospheric and solar neutrino fluxes, respectively. In this paper, regions of the three-neutrino-flavor parameter space, compatible with the existing atmospheric and solar neutrino data (including the new results from GALLEX) within the vacuum oscillation scheme, are identified.

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selected citations
These citations are derived from selected sources.
This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Citations provided by BIP!
popularity
This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
BIP!Popularity provided by BIP!
influence
This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Influence provided by BIP!
impulse
This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
BIP!Impulse provided by BIP!
9
Average
Top 10%
Top 10%
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