Oscillating Neutrinos from the Galactic Center

摘要: It has recently been demonstrated that the γ-ray emission spectrum of EGRET-identified central Galactic source 2EG J1746-2852 can be well fitted by positing these photons are generated decay π0's produced in p-p scattering at or near an energizing shock. Such also produces charged pions which leptonically. The ratio γ-rays to neutrinos accurately determined, and a well-defined potentially measurable high-energy neutrino flux Earth is unavoidable. An opportunity, therefore, detect oscillations over unprecedented scale offered this source. In paper we assess prospects for such observation with generation Cerenkov telescopes now planning stage. We determine next detectors may find oscillation signature center (GC) signal.