Echo Technique to Distinguish Flavors of Astrophysical Neutrinos
Abstract
The flavor composition of high-energy astrophysical neutrinos is a rich observable. However, present analyses cannot effectively distinguish particle showers induced by νe vs ντ. We show that this can be accomplished by measuring the intensities of the delayed, collective light emission from muon decays and neutron captures, which are, on average, greater for ντ than for νe. In conclusion, this new technique would significantly improve tests of the nature of astrophysical sources and of neutrino properties. We discuss the promising prospects for implementing it in IceCube and other detectors.
- Authors:
-
- The Ohio State Univ., Columbus, OH (United States); SLAC National Accelerator Lab., Menlo Park, CA (United States)
- The Ohio State Univ., Columbus, OH (United States); Niels Bohr Institute, Copenhagen (Denmark)
- The Ohio State Univ., Columbus, OH (United States)
- Publication Date:
- Research Org.:
- SLAC National Accelerator Laboratory (SLAC), Menlo Park, CA (United States)
- Sponsoring Org.:
- USDOE
- OSTI Identifier:
- 1526442
- Grant/Contract Number:
- AC02-76SF00515; PHY-1404311
- Resource Type:
- Accepted Manuscript
- Journal Name:
- Physical Review Letters
- Additional Journal Information:
- Journal Volume: 122; Journal Issue: 15; Journal ID: ISSN 0031-9007
- Publisher:
- American Physical Society (APS)
- Country of Publication:
- United States
- Language:
- English
- Subject:
- 79 ASTRONOMY AND ASTROPHYSICS; 43 PARTICLE ACCELERATORS
Citation Formats
Li, Shirley Weishi, Bustamante, Mauricio, and Beacom, John F. Echo Technique to Distinguish Flavors of Astrophysical Neutrinos. United States: N. p., 2019.
Web. doi:10.1103/physrevlett.122.151101.
Li, Shirley Weishi, Bustamante, Mauricio, & Beacom, John F. Echo Technique to Distinguish Flavors of Astrophysical Neutrinos. United States. https://doi.org/10.1103/physrevlett.122.151101
Li, Shirley Weishi, Bustamante, Mauricio, and Beacom, John F. Tue .
"Echo Technique to Distinguish Flavors of Astrophysical Neutrinos". United States. https://doi.org/10.1103/physrevlett.122.151101. https://www.osti.gov/servlets/purl/1526442.
@article{osti_1526442,
title = {Echo Technique to Distinguish Flavors of Astrophysical Neutrinos},
author = {Li, Shirley Weishi and Bustamante, Mauricio and Beacom, John F.},
abstractNote = {The flavor composition of high-energy astrophysical neutrinos is a rich observable. However, present analyses cannot effectively distinguish particle showers induced by νe vs ντ. We show that this can be accomplished by measuring the intensities of the delayed, collective light emission from muon decays and neutron captures, which are, on average, greater for ντ than for νe. In conclusion, this new technique would significantly improve tests of the nature of astrophysical sources and of neutrino properties. We discuss the promising prospects for implementing it in IceCube and other detectors.},
doi = {10.1103/physrevlett.122.151101},
journal = {Physical Review Letters},
number = 15,
volume = 122,
place = {United States},
year = {Tue Apr 16 00:00:00 EDT 2019},
month = {Tue Apr 16 00:00:00 EDT 2019}
}
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