Nonstandard neutrino interactions in supernovae
Abstract
Nonstandard interactions (NSI) of neutrinos with matter can significantly alter neutrino flavor evolution in supernovae with the potential to impact explosion dynamics, nucleosynthesis, and the neutrinos signal. In this paper, we explore, both numerically and analytically, the landscape of neutrino flavor transformation effects in supernovae due to NSI and find a new, heretofore unseen transformation processes can occur. These new transformations can take place with NSI strengths well below current experimental limits. Within a broad swath of NSI parameter space, we observe symmetric and standard matter-neutrino resonances for supernovae neutrinos, a transformation effect previously only seen in compact object merger scenarios; in another region of the parameter space we find the NSI can induce neutrino collective effects in scenarios where none would appear with only the standard case of neutrino oscillation physics; and in a third region the NSI can lead to the disappearance of the high density Mikheyev-Smirnov-Wolfenstein resonance. Using a variety of analytical tools, we are able to describe quantitatively the numerical results allowing us to partition the NSI parameter according to the transformation processes observed. Here our results indicate nonstandard interactions of supernova neutrinos provide a sensitive probe of beyond the Standard Model physics complementary to presentmore »
- Authors:
-
- North Carolina State University, Raleigh, NC (United States)
- Brandeis University, Waltham, MA (United States)
- Publication Date:
- Research Org.:
- North Carolina State University, Raleigh, NC (United States)
- Sponsoring Org.:
- USDOE Office of Science (SC); US Department of Education
- OSTI Identifier:
- 1536160
- Alternate Identifier(s):
- OSTI ID: 1333768
- Grant/Contract Number:
- FG02-02ER41216; SC0006417; FG02-10ER41577
- Resource Type:
- Accepted Manuscript
- Journal Name:
- Physical Review. D.
- Additional Journal Information:
- Journal Volume: 94; Journal Issue: 9; 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; 79 ASTRONOMY AND ASTROPHYSICS; neutrino interactions; novae; supernovae; neutron stars and pulsars
Citation Formats
Stapleford, Charles J., Väänänen, Daavid J., Kneller, James P., McLaughlin, Gail C., and Shapiro, Brandon T. Nonstandard neutrino interactions in supernovae. United States: N. p., 2016.
Web. doi:10.1103/physrevd.94.093007.
Stapleford, Charles J., Väänänen, Daavid J., Kneller, James P., McLaughlin, Gail C., & Shapiro, Brandon T. Nonstandard neutrino interactions in supernovae. United States. https://doi.org/10.1103/physrevd.94.093007
Stapleford, Charles J., Väänänen, Daavid J., Kneller, James P., McLaughlin, Gail C., and Shapiro, Brandon T. Tue .
"Nonstandard neutrino interactions in supernovae". United States. https://doi.org/10.1103/physrevd.94.093007. https://www.osti.gov/servlets/purl/1536160.
@article{osti_1536160,
title = {Nonstandard neutrino interactions in supernovae},
author = {Stapleford, Charles J. and Väänänen, Daavid J. and Kneller, James P. and McLaughlin, Gail C. and Shapiro, Brandon T.},
abstractNote = {Nonstandard interactions (NSI) of neutrinos with matter can significantly alter neutrino flavor evolution in supernovae with the potential to impact explosion dynamics, nucleosynthesis, and the neutrinos signal. In this paper, we explore, both numerically and analytically, the landscape of neutrino flavor transformation effects in supernovae due to NSI and find a new, heretofore unseen transformation processes can occur. These new transformations can take place with NSI strengths well below current experimental limits. Within a broad swath of NSI parameter space, we observe symmetric and standard matter-neutrino resonances for supernovae neutrinos, a transformation effect previously only seen in compact object merger scenarios; in another region of the parameter space we find the NSI can induce neutrino collective effects in scenarios where none would appear with only the standard case of neutrino oscillation physics; and in a third region the NSI can lead to the disappearance of the high density Mikheyev-Smirnov-Wolfenstein resonance. Using a variety of analytical tools, we are able to describe quantitatively the numerical results allowing us to partition the NSI parameter according to the transformation processes observed. Here our results indicate nonstandard interactions of supernova neutrinos provide a sensitive probe of beyond the Standard Model physics complementary to present and future terrestrial experiments.},
doi = {10.1103/physrevd.94.093007},
journal = {Physical Review. D.},
number = 9,
volume = 94,
place = {United States},
year = {Tue Nov 29 00:00:00 EST 2016},
month = {Tue Nov 29 00:00:00 EST 2016}
}
Web of Science
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