Search for Heavy Neutrino in K->mu nu_h(nu_h-> nu gamma) Decay at ISTRA+ Setup
ISTRA+ collaboration: V. A. Duk, V. N. Bolotov, A. A. Khudyakov, V. A., Lebedev, A. I. Makarov, V. P. Novikov, A. Yu. Polyarush, S. A. Akimenko, G., I. Britvich, A. P. Filin, A. V. Inyakin, S. A. Kholodenko, V. M. Leontiev, V., F. Obraztsov, V. A. Polyakov, V. I. Romanovsky

TL;DR
This study searches for heavy neutrinos in kaon decays, setting upper limits on their mixing parameters within specific mass and lifetime ranges, thereby constraining new physics models involving neutrino properties.
Contribution
It provides the first experimental upper limits on heavy neutrino mixing in the specified mass and lifetime range using the ISTRA+ setup.
Findings
Upper limits on |U_mu_h|^2: 5 x 10^{-5} (Majorana), 8 x 10^{-5} (Dirac)
Mass range 30-80 MeV/c^2 for heavy neutrinos
Lifetime range 10^{-11} to 10^{-9} seconds
Abstract
Heavy neutrino nu_h with m_h < 300MeV/c^2 can be effectively searched for in kaon decays. We put upper limits on mixing matrix element |U_mu_h}|^2 for radiatively decaying nu_h from K->mu nu_h (nu_h -> nu gamma) decay chain in the following parameter region: 30MeV/c^2 < m_h < 80MeV/c^2; 10^{-11}sec < tau_h < 10^{-9}sec. For the whole region |U_{mu h}|^2 < 5 x 10^{-5} for Majorana type of nu_h and | U_{\mu h}|^2 < 8 x 10^{-5} for the Dirac case.
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