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As we have pointed out in (arXiv:1806.10107 [hep-ph]), the existence of neutron dark matter decay modes n -> chi + anything, where chi is a dark matter fermion, for the solution of the neutron lifetime problem changes priorities and demands to describe the neutron lifetime tau_n = 888.0(2.0)s, measured in beam experiments and defined by the decay modes n -> p + anything, in the Standard Model (SM). The latter requires the axial coupling constant lambda to be equal to lambda = - 1.2690 (arXiv:1806.10107 [hep-ph]). Since such an axial coupling constant is excluded by experimental data reported by the PERKEO II and UCNA Collaborations, the neutron lifetime tau_n = 888.0(2.0)s can be explained only by virtue of interactions beyond the SM, namely, by the Fierz interference term of order b ~ - 10^{-2} dependent on scalar and tensor coupling constants. We give a complete analysis of all correlation coefficients of the neutron beta decays with polarized neutron, taking into account the contributions of scalar and tensor interactions beyond the SM with the Fierz interference term b ~ - 10^{-2}. We show that the obtained results agree well with the contemporary experimental data that does not prevent the neutron with the rate of the decay modes n -> p + anything, measured in beam experiments, to have dark matter decay modes n -> chi + anything.
We analyze the contributions of the one-pion-pole (OPP) exchange, caused by strong low-energy interactions, and the pseudoscalar interaction beyond the Standard Model (BSM) to the correlation coefficients of the neutron beta-decays for polarized neut
We demonstrate that the observation of neutron stars with masses greater than one solar mass places severe demands on any exotic neutron decay mode that could explain the discrepancy between beam and bottle measurements of the neutron lifetime. If th
We calculate the correlation coefficients of the electron-energy and electron-antineutrino angular distribution of the neutron beta decay with polarized electron and unpolarised neutron and proton. The calculation is carried out within the Standard M
In the standard effective V - A theory of low-energy weak interactions (i.e. in the Standard Model (SM)) we analyze the structure of the correlation coefficients S(E_e) and U(E_e), where E_e is the electron energy. These correlation coefficients were
Although well studied, the neutron still offers a unique laboratory for precise tests of Standard Model (SM) predictions. Neutron decay is free of nuclear structure corrections present in nuclear beta decays, and, with a $10^8$ times larger branching