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The observation of TeV-gamma rays of neutral pion origin from the supernovaremnant RX J1713.7-3946 might have revealed the first specific site whereprotons are accelerated to energies typical of the main component of the cosmicrays. In this letter we calculate the high-energy neutrino flux associated withthis source to be at least 40 muon-type neutrinos per kilometer-squared peryear. We perform the same calculations for other known sources of TeV-gammarays and show how neutrino observations can establish whether the TeV-gammarays emitted by blazars and supernova remnants are the decay products ofneutral pions and thus unequivocally establish the sources as cosmicaccelerators.Comment: Replaced with version published in Astrophys.

Possible High-Energy Neutrinos from the Cosmic Accelerator RX J1713.7−3946