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dc.contributor.authorTseng, JJen_US
dc.contributor.authorYeh, TWen_US
dc.contributor.authorAthar, Hen_US
dc.contributor.authorHuang, MAen_US
dc.contributor.authorLee, FFen_US
dc.contributor.authorLin, GLen_US
dc.date.accessioned2019-04-03T06:38:22Z-
dc.date.available2019-04-03T06:38:22Z-
dc.date.issued2003-09-15en_US
dc.identifier.issn2470-0010en_US
dc.identifier.urihttp://dx.doi.org/10.1103/PhysRevD.68.063003en_US
dc.identifier.urihttp://hdl.handle.net/11536/27528-
dc.description.abstractWe 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.isoen_USen_US
dc.titleEnergy spectrum of tau leptons induced by the high energy Earth-skimming neutrinosen_US
dc.typeArticleen_US
dc.identifier.doi10.1103/PhysRevD.68.063003en_US
dc.identifier.journalPHYSICAL REVIEW Den_US
dc.citation.volume68en_US
dc.citation.issue6en_US
dc.citation.spage0en_US
dc.citation.epage0en_US
dc.contributor.department物理研究所zh_TW
dc.contributor.departmentInstitute of Physicsen_US
dc.identifier.wosnumberWOS:000185830200011en_US
dc.citation.woscount31en_US
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