  This research is to determine at Earth the high-energy neutrino flux coming
from the galactic core, and from the many other accretion disks within the
galactic core. It is estimated there are 10,000 such accretion disk within the
cubic parsec of the galactic core alone and many more in the galactic core
halo. There are various neutrino detectors, such as IceCube, which can detect
energetic neutrinos. However, the direct galactic core neutrino flux is
exceptionally low, so very few neutrinos from the galactic core are measured.
We created two models to simulate the galactic core neutrino flux. To better
estimate the neutrino flux we randomly distributed the accretion disks and
generated bodies of varying sizes. This was then used to determine the
ultra-high energy neutrino flux. Since it is extremely difficult to determine
neutrino direction from interactions of neutrinos, we envision an application
where the energetic galactic core neutrinos are gravitationally focused by the
Sun with a large light collecting power of eleven to twelve orders of
magnitude. They could interact in a planet's atmosphere where the produced
showers containing energetic charged particles can produce Cherenkov rings
imageable by an orbiting spacecraft or upward going muons which can be observed
in a cosmic ray experiment. Estimating the flux will provide a general
approximation of the number of ultra-high energy neutrinos that should reach
Earth, with Earth being the overall detector. Moreover, studying the neutrinos
will provide more information on the conditions of the galactic region, and
allow characterizations of it to be formed.
