2006
DOI: 10.1103/physrevd.73.013005
|View full text |Cite
|
Sign up to set email alerts
|

Confronting mass-varying neutrinos with MiniBooNE

Abstract: We study the proposal that mass-varying neutrinos could provide an explanation for the LSND signal forν µ →ν e oscillations. We first point out that all positive oscillation signals occur in matter and that three active mass-varying neutrinos are insufficient to describe all existing neutrino data including LSND. We then examine the possibility that a model with four mass-varying neutrinos (three active and one sterile) can explain the LSND effect and remain consistent with all other neutrino data. We find tha… Show more

Help me understand this report
View preprint versions

Search citation statements

Order By: Relevance

Paper Sections

Select...
3
1
1

Citation Types

3
73
0
1

Year Published

2006
2006
2020
2020

Publication Types

Select...
6
2
1

Relationship

0
9

Authors

Journals

citations
Cited by 66 publications
(77 citation statements)
references
References 100 publications
3
73
0
1
Order By: Relevance
“…(3) one can see that w X (z) is on the same footing as ρ ′ X (z). Specifically, Wang & Garnavich (2001) argued that ρ X (z) should be preferred since it suffers less from the smearing effect (due to the multiple integrals that relate w X (z) to d L (z)) that makes constraining w X (z) extremely difficult (Maor, Brustein, & Steinhardt 2001;Barger & Marfatia 2001). Tegmark (2002) came to the same conclusion.…”
Section: Introductionmentioning
confidence: 97%
“…(3) one can see that w X (z) is on the same footing as ρ ′ X (z). Specifically, Wang & Garnavich (2001) argued that ρ X (z) should be preferred since it suffers less from the smearing effect (due to the multiple integrals that relate w X (z) to d L (z)) that makes constraining w X (z) extremely difficult (Maor, Brustein, & Steinhardt 2001;Barger & Marfatia 2001). Tegmark (2002) came to the same conclusion.…”
Section: Introductionmentioning
confidence: 97%
“…For example, the neutrino mass evolution with time can be tested in the measurement of the time delay of the neutrinos emitted from the short gamma ray bursts [33]. Another interesting possibility is to detect the neutrino mass variation in space via the neutrino oscillations [19,20,34,35,36].…”
Section: Introductionmentioning
confidence: 99%
“…Effects on neutrino oscillation [19,20,21,22,23,24,25,26,27,28] were analyzed in different scenarios. In particular, it was proposed that the Mass Varying Neutrinos phenomenology could lead to a neutrino mass dependence with baryonic density [19] through non-renormalizable operators that couple the acceleron to the baryonic matter.…”
Section: Introductionmentioning
confidence: 99%