Glashow resonance as a window into cosmic neutrino sources
Abstract
The Glashow resonance at Eν=6.3 PeV is a measure of the $$\bar{ν}$$e content of the astrophysical neutrino flux. The fractional $$\bar{ν}$$e content depends on the neutrino production model at the cosmic neutrino source, and the environment at the source. Thus, the strength of the Glashow resonance event rate is a potential window into astrophysical sources. We quantify the "Glashow resonometer" and comment on the significance that no Glashow events are observed in the IceCube three-year data.
- Authors:
-
- Univ. of Wisconsin, Madison, WI (United States)
- Vanderbilt Univ., Nashville, TN (United States)
- Univ. of Hawaii, Honolulu, HI (United States)
- Publication Date:
- Research Org.:
- Univ. of Hawaii, Honolulu, HI (United States)
- Sponsoring Org.:
- USDOE Office of Science (SC), High Energy Physics (HEP)
- OSTI Identifier:
- 1598677
- Alternate Identifier(s):
- OSTI ID: 1180298
- Grant/Contract Number:
- SC0010504; FG-02-95ER40896; FG05-85ER40226
- Resource Type:
- Accepted Manuscript
- Journal Name:
- Physical Review. D, Particles, Fields, Gravitation and Cosmology
- Additional Journal Information:
- Journal Volume: 90; Journal Issue: 12; Journal ID: ISSN 1550-7998
- Publisher:
- American Physical Society (APS)
- Country of Publication:
- United States
- Language:
- English
- Subject:
- 79 ASTRONOMY AND ASTROPHYSICS
Citation Formats
Barger, V., Fu, Lingjun, Learned, J. G., Marfatia, D., Pakvasa, S., and Weiler, T. J. Glashow resonance as a window into cosmic neutrino sources. United States: N. p., 2014.
Web. doi:10.1103/PhysRevD.90.121301.
Barger, V., Fu, Lingjun, Learned, J. G., Marfatia, D., Pakvasa, S., & Weiler, T. J. Glashow resonance as a window into cosmic neutrino sources. United States. https://doi.org/10.1103/PhysRevD.90.121301
Barger, V., Fu, Lingjun, Learned, J. G., Marfatia, D., Pakvasa, S., and Weiler, T. J. Fri .
"Glashow resonance as a window into cosmic neutrino sources". United States. https://doi.org/10.1103/PhysRevD.90.121301. https://www.osti.gov/servlets/purl/1598677.
@article{osti_1598677,
title = {Glashow resonance as a window into cosmic neutrino sources},
author = {Barger, V. and Fu, Lingjun and Learned, J. G. and Marfatia, D. and Pakvasa, S. and Weiler, T. J.},
abstractNote = {The Glashow resonance at Eν=6.3 PeV is a measure of the $\bar{ν}$e content of the astrophysical neutrino flux. The fractional $\bar{ν}$e content depends on the neutrino production model at the cosmic neutrino source, and the environment at the source. Thus, the strength of the Glashow resonance event rate is a potential window into astrophysical sources. We quantify the "Glashow resonometer" and comment on the significance that no Glashow events are observed in the IceCube three-year data.},
doi = {10.1103/PhysRevD.90.121301},
journal = {Physical Review. D, Particles, Fields, Gravitation and Cosmology},
number = 12,
volume = 90,
place = {United States},
year = {Fri Dec 12 00:00:00 EST 2014},
month = {Fri Dec 12 00:00:00 EST 2014}
}
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