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High Energy Physics - Phenomenology

arXiv:hep-ph/0401242 (hep-ph)
[Submitted on 30 Jan 2004 ]

Title: Atmospheric and galactic tau neutrinos

Title: 大气和银河tau中微子

Authors:H. Athar
Abstract: Neutrinos with energy greater than GeV are copiously produced in the p(A,p) interactions occurring in the earth atmosphere and in our galactic plane. A comparison of the tau and mu neutrino flux in the presence of neutrino oscillations from these two astrophysical sites is presented. It is pointed out that the galactic plane tau neutrino flux dominates over the downward going atmospheric tau neutrino flux at much lower energy value than that for the dominance of the mu neutrino flux from these two sites. Future prospects for possible observations of galactic tau neutrino flux are also briefly mentioned.
Abstract: 能量高于GeV的中微子在地球大气层和我们银河平面中的p(A,p)相互作用中大量产生。 在这些天体物理源的中微子振荡存在的情况下,对tau中微子和mu中微子通量进行了比较。 指出与来自这两个天体物理源的mu中微子通量占主导地位的能量值相比,银河平面的tau中微子通量在更低的能量值上就超过了向下运动的大气tau中微子通量。 也简要提到了未来可能观测银河tau中微子通量的前景。
Comments: 8 pages, 4 figures, invited talk given at CosPA 2003, 13-15 Nov, 2003, Taipei, Taiwan
Subjects: High Energy Physics - Phenomenology (hep-ph) ; Astrophysics (astro-ph)
Cite as: arXiv:hep-ph/0401242
  (or arXiv:hep-ph/0401242v1 for this version)
  https://doi.org/10.48550/arXiv.hep-ph/0401242
arXiv-issued DOI via DataCite
Journal reference: Mod.Phys.Lett. A19 (2004) 1171-1178
Related DOI: https://doi.org/10.1142/S0217732304014525
DOI(s) linking to related resources

Submission history

From: Athar Husain [view email]
[v1] Fri, 30 Jan 2004 07:08:32 UTC (32 KB)
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