 Photon brightness perturbation

The photon brightness perturbation is the fractional frequency-integrated directional energy perturbation. For a small blackbody temperature shift $\Theta =\delta T/T$, $f_1=-q{f}_0^{\prime }(q)\Theta$. Integration by parts gives $\Delta =4\Theta$. Its direction average is the photon density contrast. This temperature identification assumes a perturbation of blackbody form; the integrated brightness definition itself is more general.

// Target: cosmology.bigb