That's it: The weak interaction breaks P, C, CP, and due to the CPT theorem then also T invariance. These are all discrete symmetries of space-time, and there's no need for them to hold in nature. The only thing that's really important on a very fundamental ground is that the causality structure of space-time holds, and for this it's sufficient that the variation of the action is invariant under the part of the Poincare group that is simply connected with the neutral element of that group, and that's the proper orthochroneous Lorentz transform.
As soon as parity (spatial-reflection symmetry) is violated, a spin-1/2 particle needs not be represented necessarily by a Dirac spinor but also a Weyl spinor is sufficient, and the two kinds of Weyl spinors corresponding to the irreducible representations of the covering group of the Lorentz group, SL(2,C), labelled as the (1/2,0) and (0,1/2) representations, correspond to the left- and right-handed parts (particles of definite chirality) of the Dirac spinor ##(1\mp \gamma^5)/2 \psi##.
In the standard model the weak interaction has the famous structure (vector current minus axial vector current), and thus only the left-handed part of the neutrinos and the right-handed part of the antineutrinos couples to the "massive leptons". In the approximation of massless neutrinos, there are only left-handed neutrinos and right-handed anti-neutrinos in the game.
For massive neutrinos, there is also mixing as in the quark sector, i.e., the flavor-eigenstates are not the mass eigenstates, which gives rise to neutrino oscillations.