Neutron Oscillations to Parallel World: Earlier End to the Cosmic Ray Spectrum?

preprint2012arXivOpen access

Abstract

Present experimental data do not exclude fast oscillation of the neutron nn to its degenerate twin from a hypothetical parallel sector, the so called mirror neutron n′n'. We show that this effect brings to a remarkable modifications of the ultrahigh-energy cosmic ray spectrum testable by the present Pierre Auger Observatory (PAO) and Telescope Array (TA) detector, and the future JEM-EUSO experiment. In particular, the baryon non-conservation during UHECR propagation at large cosmological distances shifts the beginning of the GZK cutoff to lower energies, while in presence of mirror sources it may enhance the spectrum at E≳100E \gtrsim 100 EeV. As a consequence, a significant reduction of the expected diffuse cosmogenic neutrino flux is predicted.

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