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Non-unitary evolution of neutrinos in matter and the leptonic unitarity test

Abstract

We present a comprehensive study of the three-active plus NN sterile neutrino model as a framework for constraining leptonic unitarity violation induced at energy scales much lower than the electroweak scale. We formulate a perturbation theory with expansion in small unitarity violating matrix element WW while keeping (non-WW suppressed) matter effect to all orders. We show that under the same condition of sterile state masses 0.1 eV2≲mJ2≲(1−10) GeV20.1\, \text{eV}^2 \lesssim m^2_{J} \lesssim (1-10)\, \text{GeV}^2 as in vacuum, assuming typical accelerator based long-baseline neutrino oscillation experiment, one can derive a very simple form of the oscillation probability which consists only of zeroth-order terms with the unique exception of probability leaking term Cαβ\mathcal{C}_{\alpha \beta} of O(W4)\mathcal{O} (W^4). We argue, based on our explicit computation to fourth-order in WW, that all the other terms are negligibly small after taking into account the suppression due to the mass condition for sterile states, rendering the oscillation probability {\em sterile-sector model independent}. Then, we identify a limited energy region in which this suppression is evaded and the effects of order W2W^2 corrections may be observable. Its detection would provide another way, in addition to detecting Cαβ\mathcal{C}_{\alpha \beta}, to distinguish between low-scale and high-scale unitarity violation. We also solve analytically the zeroth-order system in matter with uniform density to provide a basis for numerical evaluation of non-unitary neutrino evolution.Comment: 35 content pages + 12 appendix pages, 4 figures; Several clarifying modifications to match the published versio

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