Tracing very high energy neutrinos from cosmological distances in ice

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

doi:10.1103/PhysRevD.69.033004

Tracing very high energy neutrinos from cosmological distances in ice

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

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41 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 [Formula Presented] 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 the energy loss of charged leptons. We discuss the signals of tau neutrinos in detectors such as IceCube, RICE, and ANITA.

Original language	English (US)
Journal	Physical Review D - Particles, Fields, Gravitation and Cosmology
Volume	69
Issue number	3
DOIs	https://doi.org/10.1103/PhysRevD.69.033004
State	Published - Feb 25 2004

ASJC Scopus subject areas

Nuclear and High Energy Physics
Physics and Astronomy (miscellaneous)

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10.1103/PhysRevD.69.033004

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title = "Tracing very high energy neutrinos from cosmological distances 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 [Formula Presented] 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 the energy loss of charged leptons. We discuss the signals of tau neutrinos in detectors such as IceCube, RICE, and ANITA.",

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

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AU - Reno, M. H.

AU - Sarcevic, I.

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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 [Formula Presented] 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 the energy loss of charged leptons. We discuss the 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 [Formula Presented] 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 the energy loss of charged leptons. We discuss the signals of tau neutrinos in detectors such as IceCube, RICE, and ANITA.

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Tracing very high energy neutrinos from cosmological distances in ice

Abstract

ASJC Scopus subject areas

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