Tracing very high energy tau neutrinos from cosmological sources in ice

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

Research output: Contribution to journalArticle

3 Citations (Scopus)

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 languageEnglish (US)
Pages (from-to)1204-1211
Number of pages8
JournalInternational Journal of Modern Physics A
Volume20
Issue number6
DOIs
StatePublished - Mar 10 2005

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tracing
Tracing
Neutrinos
High Energy
ice
neutrinos
energy
Energy
Neutrino Oscillations
Regeneration
transit
regeneration
leptons
Detector
astrophysics
energy dissipation
oscillations
detectors

All Science Journal Classification (ASJC) codes

  • Physics and Astronomy(all)
  • Mathematical Physics
  • Nuclear and High Energy Physics

Cite this

Jones, J. ; Mocioiu, Irina ; Sarcevic, I. ; Reno, M. H. / Tracing very high energy tau neutrinos from cosmological sources in ice. In: International Journal of Modern Physics A. 2005 ; Vol. 20, No. 6. pp. 1204-1211.
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Tracing very high energy tau neutrinos from cosmological sources in ice. / Jones, J.; Mocioiu, Irina; Sarcevic, I.; Reno, M. H.

In: International Journal of Modern Physics A, Vol. 20, No. 6, 10.03.2005, p. 1204-1211.

Research output: Contribution to journalArticle

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