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Cited by 317

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Atmospheric neutrino flux above 1 GeV

Open access
Agrawal, Vivek, Gaisser, T. K., Lipari, Paolo, Stanev, Todor·1996·Physical Review D

Abstract

In this paper we extend an earlier calculation of the flux of atmospheric neutrinos to higher energy. The earlier calculation of the neutrino flux below 3 GeV has been used for calculation of the rate of contained neutrino interactions in deep underground detectors. The fluxes are needed up to neutrino energies of 10 TeV to calculate the expected rate of neutrino-induced muons passing into and through large, deep detectors. We compare our results with several other calculations, and we evaluate the uncertainty in the rate of neutrino-induced muons due to uncertainties in the neutrino flux. \textcopyright{} 1996 The American Physical Society.

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Metadata

Authors
Agrawal, V., Gaisser, T. K., Lipari, P., & Stanev, T.
Venue
Physical Review D
Published
1996-02-01
Volume
53
Issue
3
Pages
1314-1323
ISSN
  • 0556-2821 (ISSN-L)
  • 1089-4918
OpenAlex
W2129766080
Cited by
317
References
1
FWCI
13.53
Type
journal article
Language
en
Open access
green

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CoChat. (2026). Citation check: Atmospheric neutrino flux above 1 GeV. https://app.cochat.ai/papers/10.1103/physrevd.53.1314
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Agrawal, V., Gaisser, T. K., Lipari, P., & Stanev, T. (1996). Atmospheric neutrino flux above 1 GeV. Physical Review D. https://doi.org/10.1103/physrevd.53.1314

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