“…However, with the advent of TeV scale accelerators, we shall soon have access to energies which are much larger than the symmetry breaking scale (say, the W mass) which may act as infrared cutoff and thus give rise to parametrically large infrared logarithms in the energy dependence, in addition to the ones of collinear origin. That this is indeed the case was first remarked in the late nineties [17] and soon applied to inclusive observables [18]. The failure of the BN theorem is due again to the nonabelian nature of electroweak theory, where now no averaging over flavour is possible, because the initial state consists of electrons, protons, and so on, each of them having a nontrivial weak isospin charge.…”