We analyze the correlation coefficient T (Ee), which was introduced by Ebel and Feldman (Nucl. Phys. 4, 213 (1957)). The correlation coefficient T (Ee) is induced by the correlation structure ( ξn • kν )( ke • ξe)/EeEν, where ξn,e are unit spin-polarization vectors of the neutron and electron, and (Ee,ν , ke,ν) are energies and 3-momenta of the electron and antineutrino. Such a correlation structure is invariant under discrete P, C and T symmetries. The correlation coefficient T (Ee), calculated to leading order in the large nucleon mass mN expansion, is equal to T (Ee) = −2gA(1 + gA)/(1 + 3g 2 A ) = −B0, i.e. of order |T (Ee)| ∼ 1, where gA is the axial coupling constant. Within the Standard Model (SM) we describe the correlation coefficient T (Ee) at the level of 10 −3 by taking into the radiative corrections of order O(α/π) or the outer model-independent radiative corrections, where α is the fine-structure constant, and the corrections of order O(Ee/mN ), caused by weak magnetism and proton recoil. We calculate also the contributions of interactions beyond the SM, including the contributions of the second class currents.