The future of high-energy astrophysical neutrino flavor measurements

Song, Ningqiang; Li, Shirley Weishi; Argüelles, Carlos A.; Bustamante, Mauricio; Vincent, Aaron C.

doi:10.1088/1475-7516/2021/04/054

The future of high-energy astrophysical neutrino flavor measurements

Journal Article · Tue Apr 20 00:00:00 EDT 2021 · Journal of Cosmology and Astroparticle Physics

DOI:https://doi.org/10.1088/1475-7516/2021/04/054· OSTI ID:1798649

Song, Ningqiang ^[1]; Li, Shirley Weishi ^[2]; Argüelles, Carlos A. ^[3]; Bustamante, Mauricio ^[4]; Vincent, Aaron C. ^[1]

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.

In this paper, 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.

View Accepted Manuscript (DOE)

Research Organization:: Fermi National Accelerator Laboratory (FNAL), Batavia, IL (United States); SLAC National Accelerator Laboratory (SLAC), Menlo Park, CA (United States)

Sponsoring Organization:: USDOE Office of Science (SC), Basic Energy Sciences (BES); USDOE Office of Science (SC), High Energy Physics (HEP); Villum Fonden

Grant/Contract Number:: AC02-07CH11359; AC02-76SF00515

OSTI ID:: 1798649

Alternate ID(s):: OSTI ID: 1831478
OSTI ID: 23181607

Report Number(s):: FERMILAB-PUB--21-006-T; arXiv:2012.12893

Journal Information:: Journal of Cosmology and Astroparticle Physics, Journal Name: Journal of Cosmology and Astroparticle Physics Journal Issue: 04 Vol. 2021; ISSN 1475-7516

Publisher:: Institute of Physics (IOP)Copyright Statement

Country of Publication:: United States

Language:: English

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Cosmic Neutrinos and the Cosmic-Ray Accelerator TXS 0506+056 Halzen, Francis Proceedings of 36th International Cosmic Ray Conference — PoS(ICRC2019) https://doi.org/10.22323/1.358.0021	conference	August 2019
Fundamental Physics with High-Energy Astrophysical Neutrinos Today and in the Future Bustamante, Mauricio; Arguelles, Carlos; Kheirandish, Ali Proceedings of 36th International Cosmic Ray Conference — PoS(ICRC2019) https://doi.org/10.22323/1.358.0849	conference	July 2019
Calibration LEDs in the IceCube Upgrade DEgg modules Ishihara, Aya; Kiriki, Ayumi Proceedings of 36th International Cosmic Ray Conference — PoS(ICRC2019) https://doi.org/10.22323/1.358.0923	conference	July 2019
Electronics Development for the New Photo-Detectors (PDOM and D-Egg) for IceCube-Upgrade Nagai, Ryo; Ishihara, Aya Proceedings of 36th International Cosmic Ray Conference — PoS(ICRC2019) https://doi.org/10.22323/1.358.0966	conference	July 2019
The Baikal-GVD neutrino telescope: First results of multi-messenger study Simkovic, Fedor; Avrorin, A. D.; Avrorin, A. V. Proceedings of 36th International Cosmic Ray Conference — PoS(ICRC2019) https://doi.org/10.22323/1.358.1013	conference	July 2019
Measurement of the diffuse astrophysical muon-neutrino spectrum with ten years of IceCube data Stettner, Joeran Proceedings of 36th International Cosmic Ray Conference — PoS(ICRC2019) https://doi.org/10.22323/1.358.1017	conference	July 2019
The IceCube Upgrade - Design and Science Goals Ishihara, Aya Proceedings of 36th International Cosmic Ray Conference — PoS(ICRC2019) https://doi.org/10.22323/1.358.1031	conference	July 2019
Baikal-GVD: status and first results Safronov, Grigory; Avrorin, A. D.; Avrorin, A. V. Proceedings of 40th International Conference on High Energy physics — PoS(ICHEP2020) https://doi.org/10.22323/1.390.0606	conference	December 2020
Neutrino Telescopes and High-Energy Cosmic Neutrinos Palladino, Andrea; Spurio, Maurizio; Vissani, Francesco Universe, Vol. 6, Issue 2 https://doi.org/10.3390/universe6020030	journal	February 2020
Observation and Characterization of a Cosmic muon Neutrino flux from the Northern Hemisphere Using six Years of Icecube data Aartsen, M. G.; Abraham, K.; Ackermann, M. The Astrophysical Journal, Vol. 833, Issue 1 https://doi.org/10.3847/0004-637X/833/1/3	journal	December 2016
A New Generation of Standard Solar Models Vinyoles, Núria; Serenelli, Aldo M.; Villante, Francesco L. The Astrophysical Journal, Vol. 835, Issue 2 https://doi.org/10.3847/1538-4357/835/2/202	journal	January 2017
A Search for Neutrino Point-source Populations in 7 yr of IceCube Data with Neutrino-count Statistics Aartsen, M. G.; Ackermann, M.; Adams, J. The Astrophysical Journal, Vol. 893, Issue 2 https://doi.org/10.3847/1538-4357/ab7af9	journal	April 2020

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