Abstract
The oscillation probability over short baseline (~km) would be negligible in case the mixing matrix for three active neutrinos is unitary. However, in case of non-unitary mixing of three neutrinos, this probability would be non-negligible due to the so-called "zero distance" effect. Hence, the near detector of the accelerator experiments such as NOA can provide strong constraints on the parameters of the non-unitary mixing with very large statistics. By analyzing the NOA near detector data we find that the non-unitary mixing does not improve fits to the or events over the standard unitary mixing. This leads to constraints on the non-unitary parameters: , and at 90\% C.L. A combined analysis with the near and far detector data does not change these constraints significantly.
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