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Title: 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:
 [1];  [2];  [3];  [3];  [3];  [2]
  1. Univ. of Wisconsin, Madison, WI (United States)
  2. Vanderbilt Univ., Nashville, TN (United States)
  3. 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}
}

Journal Article:

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Cited by: 46 works
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