Full metadata record
DC Field | Value | Language |
---|---|---|
dc.contributor.author | Tseng, JJ | en_US |
dc.contributor.author | Yeh, TW | en_US |
dc.contributor.author | Athar, H | en_US |
dc.contributor.author | Huang, MA | en_US |
dc.contributor.author | Lee, FF | en_US |
dc.contributor.author | Lin, GL | en_US |
dc.date.accessioned | 2019-04-03T06:38:22Z | - |
dc.date.available | 2019-04-03T06:38:22Z | - |
dc.date.issued | 2003-09-15 | en_US |
dc.identifier.issn | 2470-0010 | en_US |
dc.identifier.uri | http://dx.doi.org/10.1103/PhysRevD.68.063003 | en_US |
dc.identifier.uri | http://hdl.handle.net/11536/27528 | - |
dc.description.abstract | We present a semianalytic calculation of the tau-lepton flux emerging from the Earth induced by incident high energy neutrinos interacting inside the Earth for 10(5)less than or equal toE(nu)/GeVless than or equal to10(10). We obtain results for the energy dependence of the tau-lepton flux coming from the Earth-skimming neutrinos, because of the neutrino-nucleon charged-current scattering as well as the resonant (nu) over bar (e)e(-) scattering. We illustrate our results for several anticipated high energy astrophysical neutrino sources such as the active galactic nuclei, the gamma-ray bursts, and the Greisen-Zatsepin-Kuzmin neutrino fluxes. The tau-lepton fluxes resulting from rock-skimming and ocean-skimming neutrinos are compared. Such comparisons can render useful information about the spectral indices of incident neutrino fluxes. | en_US |
dc.language.iso | en_US | en_US |
dc.title | Energy spectrum of tau leptons induced by the high energy Earth-skimming neutrinos | en_US |
dc.type | Article | en_US |
dc.identifier.doi | 10.1103/PhysRevD.68.063003 | en_US |
dc.identifier.journal | PHYSICAL REVIEW D | en_US |
dc.citation.volume | 68 | en_US |
dc.citation.issue | 6 | en_US |
dc.citation.spage | 0 | en_US |
dc.citation.epage | 0 | en_US |
dc.contributor.department | 物理研究所 | zh_TW |
dc.contributor.department | Institute of Physics | en_US |
dc.identifier.wosnumber | WOS:000185830200011 | en_US |
dc.citation.woscount | 31 | en_US |
Appears in Collections: | Articles |
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