Tracing very high energy tau neutrinos from cosmological sources in ice

J. Jones; I. Mocioiu; I. Sarcevic; M. H. Reno

doi:10.1142/S0217751X05024092

Tracing very high energy tau neutrinos from cosmological sources in ice

J. Jones, I. Mocioiu, I. Sarcevic, M. H. Reno

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3 Scopus citations

Abstract

Astrophysical sources of ultrahigh energy neutrinos yield tau neutrino fluxes due to neutrino oscillations. We study in detail the contribution of tau neutrinos with energies above 10⁶ GeV relative to the contribution of the other flavors. We consider several different initial neutrino fluxes and include tau neutrino regeneration in transit through the Earth and energy loss of charged leptons. We discuss signals of tau neutrinos in detectors such as IceCube, RICE and ANITA.

Original language	English (US)
Pages (from-to)	1204-1211
Number of pages	8
Journal	International Journal of Modern Physics A
Volume	20
Issue number	6
DOIs	https://doi.org/10.1142/S0217751X05024092
State	Published - Mar 10 2005

ASJC Scopus subject areas

Atomic and Molecular Physics, and Optics
Nuclear and High Energy Physics
Astronomy and Astrophysics

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title = "Tracing very high energy tau neutrinos from cosmological sources in ice",

abstract = "Astrophysical sources of ultrahigh energy neutrinos yield tau neutrino fluxes due to neutrino oscillations. We study in detail the contribution of tau neutrinos with energies above 106 GeV relative to the contribution of the other flavors. We consider several different initial neutrino fluxes and include tau neutrino regeneration in transit through the Earth and energy loss of charged leptons. We discuss signals of tau neutrinos in detectors such as IceCube, RICE and ANITA.",

author = "J. Jones and I. Mocioiu and I. Sarcevic and Reno, {M. H.}",

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AU - Jones, J.

AU - Mocioiu, I.

AU - Sarcevic, I.

AU - Reno, M. H.

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Y1 - 2005/3/10

N2 - Astrophysical sources of ultrahigh energy neutrinos yield tau neutrino fluxes due to neutrino oscillations. We study in detail the contribution of tau neutrinos with energies above 106 GeV relative to the contribution of the other flavors. We consider several different initial neutrino fluxes and include tau neutrino regeneration in transit through the Earth and energy loss of charged leptons. We discuss signals of tau neutrinos in detectors such as IceCube, RICE and ANITA.

AB - Astrophysical sources of ultrahigh energy neutrinos yield tau neutrino fluxes due to neutrino oscillations. We study in detail the contribution of tau neutrinos with energies above 106 GeV relative to the contribution of the other flavors. We consider several different initial neutrino fluxes and include tau neutrino regeneration in transit through the Earth and energy loss of charged leptons. We discuss signals of tau neutrinos in detectors such as IceCube, RICE and ANITA.

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Tracing very high energy tau neutrinos from cosmological sources in ice

Abstract

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