High energy neutrinos from CYG X-3

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Companion Stars, Cosmic Ray Showers, Gamma Rays, Neutrinos, Radiation Detectors, X Ray Sources, Particle Production, Photons, Stellar Models

Scientific paper

Assuming that the UHE air showers from Cyg X-3 are produced by photons, the expected neutrino emission is calculated from a model which produces the (GAMMA)-rays in the atmosphere of the Cyg X-3 companion. The possibility of detecting such neutrinos in underground detectors is discussed. The constraints that such a signal places on the use of this model in other particle production scenarios is also discussed.

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