Galactic and extragalactic high energy neutrinosEstimates of fluxes from cosmic diffuse sources are made using the generic relationship between secondary gammas and neutrinos and using recent cosmic gamma-ray satellite observations. A quantitative estimate of the observability above the atmospheric background of 1-10 TeV neutrinos from the inner Galaxy for a DUMAND type detector is then given.
Document ID
19810028115
Acquisition Source
Legacy CDMS
Document Type
Conference Proceedings
Authors
Stecker, F. W. (NASA Goddard Space Flight Center Laboratory for High Energy Astrophysics, Greenbelt, Md., United States)
Shapiro, M. M. (NASA Goddard Space Flight Center Greenbelt, MD, United States)
Silberberg, R. (U.S. Navy, Naval Research Laboratory, Washington D.C., United States)