The null shear is the symmetric trace-free part . It changes the shape of a transverse beam while preserving its area to first order.
For an affine null congruence in four spacetime dimensions with a parallel-transported screen, the displayed equation follows by taking the symmetric trace-free part of the Sachs optical equations. The Ricci contribution to the optical tidal tensor is , so it changes the expansion but contributes no screen-trace-free source. The projected Weyl tensor supplies the tidal source of shear.

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  1. Optical tensor
  2. Screen-space projector
  3. Null geodesic congruence
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