Scalar Nonstandard Interactions in Neutrino Oscillation
Abstract
The scalar nonstandard interactions (NSI) can also introduce matter effect for neutrino oscillation in a medium. Especially the recent Borexino data prefer nonzero scalar NSI, ηee = -0.16. In contrast to the conventional vector NSI, the scalar type contributes as a correction to the neutrino mass matrix rather than the matter potential. Consequently, the scalar matter effect is energy independent while the vector one scales linearly with neutrino energy. This leads to significantly different phenomenological consequences in reactor, solar, atmospheric, and accelerator neutrino oscillations. A synergy of different types of experiments, especially those with matter density variation, is necessary to identify the scalar NSI and guarantee the measurement of CP violation at accelerator experiments.
- Authors:
- Publication Date:
- Research Org.:
- Fermi National Accelerator Lab. (FNAL), Batavia, IL (United States)
- Sponsoring Org.:
- USDOE Office of Science (SC), High Energy Physics (HEP)
- OSTI Identifier:
- 1523323
- Alternate Identifier(s):
- OSTI ID: 1488603
- Report Number(s):
- arXiv:1812.08376; IPMU18-0206; FERMILAB-PUB-18-487-T
Journal ID: ISSN 0031-9007; PRLTAO; 211801
- Grant/Contract Number:
- AC02-07CH11359
- Resource Type:
- Published Article
- Journal Name:
- Physical Review Letters
- Additional Journal Information:
- Journal Name: Physical Review Letters Journal Volume: 122 Journal Issue: 21; Journal ID: ISSN 0031-9007
- Publisher:
- American Physical Society
- Country of Publication:
- United States
- Language:
- English
- Subject:
- 72 PHYSICS OF ELEMENTARY PARTICLES AND FIELDS
Citation Formats
Ge, Shao-Feng, and Parke, Stephen J. Scalar Nonstandard Interactions in Neutrino Oscillation. United States: N. p., 2019.
Web. doi:10.1103/PhysRevLett.122.211801.
Ge, Shao-Feng, & Parke, Stephen J. Scalar Nonstandard Interactions in Neutrino Oscillation. United States. https://doi.org/10.1103/PhysRevLett.122.211801
Ge, Shao-Feng, and Parke, Stephen J. Wed .
"Scalar Nonstandard Interactions in Neutrino Oscillation". United States. https://doi.org/10.1103/PhysRevLett.122.211801.
@article{osti_1523323,
title = {Scalar Nonstandard Interactions in Neutrino Oscillation},
author = {Ge, Shao-Feng and Parke, Stephen J.},
abstractNote = {The scalar nonstandard interactions (NSI) can also introduce matter effect for neutrino oscillation in a medium. Especially the recent Borexino data prefer nonzero scalar NSI, ηee = -0.16. In contrast to the conventional vector NSI, the scalar type contributes as a correction to the neutrino mass matrix rather than the matter potential. Consequently, the scalar matter effect is energy independent while the vector one scales linearly with neutrino energy. This leads to significantly different phenomenological consequences in reactor, solar, atmospheric, and accelerator neutrino oscillations. A synergy of different types of experiments, especially those with matter density variation, is necessary to identify the scalar NSI and guarantee the measurement of CP violation at accelerator experiments.},
doi = {10.1103/PhysRevLett.122.211801},
journal = {Physical Review Letters},
number = 21,
volume = 122,
place = {United States},
year = {Wed May 29 00:00:00 EDT 2019},
month = {Wed May 29 00:00:00 EDT 2019}
}
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Cited by: 27 works
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Figures / Tables:
Figure 1: The effect of the scalar NSI on the reactor antineutrino oscillation probabilities at (a) Daya Bay and (b) JUNO.
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