The tensor normalization with unit-norm polarization tensors identifies the canonically normalized real scalar for each helicity as . The two polarization actions are independent and have precisely the massless scalar normalization, so the vacuum fluctuations derived in the introductory solution apply to each of them:
In the isotropic Bunch-Davies vacuum, the independent helicities have no cross correlation. Translation invariance gives the wavevector delta function, and the dimensionless-spectrum convention gives
This is power per polarization in the printed metric convention and unit-norm polarization basis. Summing polarizations or quoting a spectrum for changes normalization factors; neither operation belongs in the displayed per-polarization .