XXth International Conference on Neutrino Physics and Astrophysics
Expected Performance of a Neutrino Telescope
for Seeing AGN/GC Behind a Mountain
We study the expected performance of building a neutrino telescope,
which targets at energy greater than 10^14 eV utilizing a mountain
to interact with neutrinos. The telescope's efficiency in converting
neutrinos into leptons is first examined. Then using a potential site
on the Big Island of Hawaii, we estimate the acceptance of the
proposed detector. The neutrino flux limit at event rate 0.3/year/half
decade of energy is estimated to be comparable to that of AMANDA
neutrino flux limit at above 10^16 eV.
Powerpoint Version of Poster.