1Dropping the λ/2 at a denser-medium reflection. Every bright and dark condition inverts with it.
2Reading a sin θ = nλ as a maximum. For one slit it locates the minima; for two slits d sin θ = nλ is a maximum.
3Adding intensities for coherent beams. Add amplitudes and square, or the dark fringe never reaches zero.
4Quoting the vacuum wavelength inside a liquid. In a medium λ → λ/n, and β shrinks with it.