1986
DOI: 10.1103/physrevlett.57.2897
|View full text |Cite
|
Sign up to set email alerts
|

Limits toνμ,νeντOscillations and

Help me understand this report

Search citation statements

Order By: Relevance

Paper Sections

Select...
2
1
1
1

Citation Types

1
68
1

Year Published

1995
1995
2017
2017

Publication Types

Select...
5
4

Relationship

0
9

Authors

Journals

citations
Cited by 199 publications
(70 citation statements)
references
References 31 publications
1
68
1
Order By: Relevance
“…With regard to the constraints on each individual |U µi | 2 , the fourth equation of [5] [36]. We must note, however, that the precise translation from the constraints obtained by using the (3 + 1) model to the ones obtainable by our generic (3+N ) model requires great care.…”
Section: Jhep02(2017)114mentioning
confidence: 99%
“…With regard to the constraints on each individual |U µi | 2 , the fourth equation of [5] [36]. We must note, however, that the precise translation from the constraints obtained by using the (3 + 1) model to the ones obtainable by our generic (3+N ) model requires great care.…”
Section: Jhep02(2017)114mentioning
confidence: 99%
“…Neutrino flavor oscillations [26] represent a viable solution to the so-called solar neutrino problem [27] and to the atmospheric neutrino anomaly [28]. This phenomenon can also be probed at accelerators [29][30][31][32][33][34] and reactors [35][36][37][38]. The flavor survival probability of a neutrino with energy E ν , at a distance L from the source is…”
Section: Probing Flavor Oscillationsmentioning
confidence: 99%
“…In this framework, accelerator experiments provide strong bounds on the mixing between ν e and ν µ [5], as well as between ν τ and ν µ [6].…”
Section: Introductionmentioning
confidence: 99%