The future of high-energy astrophysical neutrino flavor measurements
Abstract
We critically examine the ability of future neutrino telescopes, including Baikal-GVD, KM3NeT, P-ONE, TAMBO, and IceCube-Gen2, to determine the flavor composition of high-energy astrophysical neutrinos in light of data from next-generation of neutrino oscillation experiments including JUNO, DUNE, and Hyper-Kamiokande. By 2040, the region of allowed flavor composition at Earth will shrink ten-fold, and the flavor composition at the astrophysical sources of the neutrinos will be inferred to within 6%, enough to pinpoint the dominant neutrino production mechanism and to identify possible sub-dominant mechanisms. These conclusions hold even in the nonstandard scenario where neutrino mixing is non-unitary, a scenario that will be probed in next-generation experiments such as the IceCube-Upgrade. As an illustration, we show that future experiments are sensitive to decay rates of the heavier neutrinos to below 1.8 × 10-5 (m/eV) s-1 at 95% credibility by 2040.
- Authors:
-
- Queen's Univ., Kingston, ON (Canada); Arthur B. McDonald Canadian Astroparticle Physics Research Institute, Kingston ON (Canada); Perimeter Inst. for Theoretical Physics, Waterloo, ON (Canada)
- SLAC National Accelerator Lab., Menlo Park, CA (United States); Fermi National Accelerator Lab. (FNAL), Batavia, IL (United States)
- Harvard Univ., Cambridge, MA (United States)
- Univ. of Copenhagen (Denmark). The Niels Bohr Inst.
- Publication Date:
- Research Org.:
- SLAC National Accelerator Laboratory (SLAC), Menlo Park, CA (United States); Fermi National Accelerator Laboratory (FNAL), Batavia, IL (United States)
- Sponsoring Org.:
- USDOE Office of Science (SC), Basic Energy Sciences (BES); Villum Foundation; USDOE Office of Science (SC), High Energy Physics (HEP)
- OSTI Identifier:
- 1798649
- Alternate Identifier(s):
- OSTI ID: 1831478
- Report Number(s):
- FERMILAB-PUB-21-006-T; arXiv:2012.12893
Journal ID: ISSN 1475-7516; TRN: US2210706
- Grant/Contract Number:
- AC02-76SF00515; AC02-07CH11359; 13164; 29388
- Resource Type:
- Accepted Manuscript
- Journal Name:
- Journal of Cosmology and Astroparticle Physics
- Additional Journal Information:
- Journal Volume: 2021; Journal Issue: 04; Journal ID: ISSN 1475-7516
- Publisher:
- Institute of Physics (IOP)
- Country of Publication:
- United States
- Language:
- English
- Subject:
- 72 PHYSICS OF ELEMENTARY PARTICLES AND FIELDS; 79 ASTRONOMY AND ASTROPHYSICS
Citation Formats
Song, Ningqiang, Li, Shirley Weishi, Argüelles, Carlos A., Bustamante, Mauricio, and Vincent, Aaron C. The future of high-energy astrophysical neutrino flavor measurements. United States: N. p., 2021.
Web. doi:10.1088/1475-7516/2021/04/054.
Song, Ningqiang, Li, Shirley Weishi, Argüelles, Carlos A., Bustamante, Mauricio, & Vincent, Aaron C. The future of high-energy astrophysical neutrino flavor measurements. United States. https://doi.org/10.1088/1475-7516/2021/04/054
Song, Ningqiang, Li, Shirley Weishi, Argüelles, Carlos A., Bustamante, Mauricio, and Vincent, Aaron C. Tue .
"The future of high-energy astrophysical neutrino flavor measurements". United States. https://doi.org/10.1088/1475-7516/2021/04/054. https://www.osti.gov/servlets/purl/1798649.
@article{osti_1798649,
title = {The future of high-energy astrophysical neutrino flavor measurements},
author = {Song, Ningqiang and Li, Shirley Weishi and Argüelles, Carlos A. and Bustamante, Mauricio and Vincent, Aaron C.},
abstractNote = {We critically examine the ability of future neutrino telescopes, including Baikal-GVD, KM3NeT, P-ONE, TAMBO, and IceCube-Gen2, to determine the flavor composition of high-energy astrophysical neutrinos in light of data from next-generation of neutrino oscillation experiments including JUNO, DUNE, and Hyper-Kamiokande. By 2040, the region of allowed flavor composition at Earth will shrink ten-fold, and the flavor composition at the astrophysical sources of the neutrinos will be inferred to within 6%, enough to pinpoint the dominant neutrino production mechanism and to identify possible sub-dominant mechanisms. These conclusions hold even in the nonstandard scenario where neutrino mixing is non-unitary, a scenario that will be probed in next-generation experiments such as the IceCube-Upgrade. As an illustration, we show that future experiments are sensitive to decay rates of the heavier neutrinos to below 1.8 × 10-5 (m/eV) s-1 at 95% credibility by 2040.},
doi = {10.1088/1475-7516/2021/04/054},
journal = {Journal of Cosmology and Astroparticle Physics},
number = 04,
volume = 2021,
place = {United States},
year = {Tue Apr 20 00:00:00 EDT 2021},
month = {Tue Apr 20 00:00:00 EDT 2021}
}
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