A possible shortcut for neutron-antineutron oscillation through mirror world

Existing bounds on the neutron-antineutron mass mixing, Enn transition probability, Pnn(t)<(t/0.1s)2x10-18 or so, where t is the neutron flight time. Here we propose a new mechanism of n-n transition which is not induced by direct mass mixing Enn but is mediated instead by the neutron mass mixings with the hypothetical states of mirror neutron n ' and mirror antineutron n'. The latter can be as large as Enn ' ,Enn' similar to 10-15 eV or so, without contradicting present experimental limits and nuclear stability bounds. The probabilities of n-n ' and n-n' transitions, Pnn ' and Pnn', depend on environmental conditions in mirror sector, and they can be resonantly amplified by applying the magnetic field of the proper value. This opens up a possibility of n-n transition with the probability Pnnsimilar or equal to Pnn' Pnn' which can reach the values similar to 10-8 or even larger. For finding this effect in real experiments, the magnetic field should not be suppressed but properly varied. These mixings can be induced by new physics at the scale of few TeV which may also originate a new low scale co-baryogenesis mechanism between ordinary and mirror sectors.

Automated summary

A new mechanism for n-n transition is proposed, mediated by mixings between neutron and hypothetical states of mirror neutron and mirror antineutron. The transition probabilities depend on environmental conditions and can be resonantly amplified by applying a magnetic field. These mixings may be induced by new physics at the scale of few TeV, potentially leading to co-baryogenesis between different sectors.