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- W3000625025 abstract "The angular distribution of muons observed deep underground (10788 ft, or 8.89 ifmmodetimeselsetexttimesfi{} ${10}^{5}$ g ${mathrm{cm}}^{ensuremath{-}2}$ standard rock) has been measured with a ${174ensuremath{-}mathrm{m}}^{2}$ liquid scintillation detector in conjunction with 48 384 neon flash tubes. The data are fitted by a curve giving the vertical intensity of muons vs vertical depth ${h}_{0}$ as ${I}_{vensuremath{mu}}({h}_{0})=A mathrm{exp}(frac{ensuremath{-}{h}_{0}}{ensuremath{lambda}})+{I}_{vensuremath{mu}}^{(ensuremath{nu})}$, where $A=(2.26ifmmodepmelsetextpmfi{}0.16)ifmmodetimeselsetexttimesfi{}{10}^{ensuremath{-}6}$ ${mathrm{cm}}^{ensuremath{-}2}$ ${mathrm{sec}}^{ensuremath{-}1}$ ${mathrm{sr}}^{ensuremath{-}1}$, and $ensuremath{gamma}=(7.58ifmmodepmelsetextpmfi{}0.09)ifmmodetimeselsetexttimesfi{}{10}^{4}$ g ${mathrm{cm}}^{ensuremath{-}2}$. The constant term, representing the measured depth-independent flux of muons produced in the surrounding rock by interactions of cosmic-ray neutrinos generated in the earth's atmosphere, has the value ${I}_{vensuremath{mu}}^{(ensuremath{nu})}=(2.23ifmmodepmelsetextpmfi{}0.20)ifmmodetimeselsetexttimesfi{}{10}^{ensuremath{-}13}$ ${mathrm{cm}}^{ensuremath{-}2}$ ${mathrm{sec}}^{ensuremath{-}1}$ ${mathrm{sr}}^{ensuremath{-}1}$. This observed flux is in fair agreement with that predicted assuming a cosmic-ray neutrino flux which is a composite of several theoretical estimates. Thus the flux of muons from extraterrestrial neutrinos is ${10}^{ensuremath{-}13}$ ${mathrm{cm}}^{ensuremath{-}2}$ ${mathrm{sec}}^{ensuremath{-}1}$ ${mathrm{sr}}^{ensuremath{-}1}$." @default.
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- W3000625025 date "1991-01-01" @default.
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- W3000625025 title "Cosmic-ray muon fluxes deep underground: Intensity vs depth, and the neutrino-induced component" @default.
- W3000625025 doi "https://doi.org/10.1142/9789814343060_0037" @default.
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