Galactic dark matter population as the source of neutrino masses
Abstract
In this study, we propose that neutrino masses can be zero in vacuo and may be generated by the local distribution of dark matter through a feeble long range scalar force. We discuss potential phenomenological constraints and implications of this framework. Our model typically implies that the cosmic neutrino background left over from the Big Bang is mostly absent in our Galactic neighborhood. Hence, a positive detection signal from future proposed experiments, such as PTOLEMY, could in principle falsify our scenario.
- Authors:
- Publication Date:
- Research Org.:
- Brookhaven National Lab. (BNL), Upton, NY (United States)
- Sponsoring Org.:
- USDOE Office of Science (SC), Workforce Development for Teachers and Scientists (WDTS); USDOE Office of Science (SC), High Energy Physics (HEP)
- OSTI Identifier:
- 1460034
- Alternate Identifier(s):
- OSTI ID: 1456886
- Report Number(s):
- BNL-205794-2018-JAAM
Journal ID: ISSN 2470-0010; PRVDAQ; 021301
- Grant/Contract Number:
- SC0012704; SC0017988
- Resource Type:
- Published Article
- Journal Name:
- Physical Review D
- Additional Journal Information:
- Journal Name: Physical Review D Journal Volume: 98 Journal Issue: 2; Journal ID: ISSN 2470-0010
- Publisher:
- American Physical Society (APS)
- Country of Publication:
- United States
- Language:
- English
- Subject:
- 72 PHYSICS OF ELEMENTARY PARTICLES AND FIELDS; mass; dark matter; neutrino; paticle physics; PTOLEMY; scalar; SM; DM; phenomenology; standard model
Citation Formats
Davoudiasl, Hooman, Mohlabeng, Gopolang, and Sullivan, Matthew. Galactic dark matter population as the source of neutrino masses. United States: N. p., 2018.
Web. doi:10.1103/PhysRevD.98.021301.
Davoudiasl, Hooman, Mohlabeng, Gopolang, & Sullivan, Matthew. Galactic dark matter population as the source of neutrino masses. United States. https://doi.org/10.1103/PhysRevD.98.021301
Davoudiasl, Hooman, Mohlabeng, Gopolang, and Sullivan, Matthew. Thu .
"Galactic dark matter population as the source of neutrino masses". United States. https://doi.org/10.1103/PhysRevD.98.021301.
@article{osti_1460034,
title = {Galactic dark matter population as the source of neutrino masses},
author = {Davoudiasl, Hooman and Mohlabeng, Gopolang and Sullivan, Matthew},
abstractNote = {In this study, we propose that neutrino masses can be zero in vacuo and may be generated by the local distribution of dark matter through a feeble long range scalar force. We discuss potential phenomenological constraints and implications of this framework. Our model typically implies that the cosmic neutrino background left over from the Big Bang is mostly absent in our Galactic neighborhood. Hence, a positive detection signal from future proposed experiments, such as PTOLEMY, could in principle falsify our scenario.},
doi = {10.1103/PhysRevD.98.021301},
journal = {Physical Review D},
number = 2,
volume = 98,
place = {United States},
year = {2018},
month = {7}
}
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https://doi.org/10.1103/PhysRevD.98.021301
https://doi.org/10.1103/PhysRevD.98.021301
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Cited by: 4 works
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Works referencing / citing this record:
Mononeutrino at DUNE: New signals from neutrinophilic thermal dark matter
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Scalar Nonstandard Interactions in Neutrino Oscillation
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