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| | Kerr Black Holes, Ch.5. Petrov Types (Site not responding. Last check: 2007-11-07) |
 | | The type of a spacetime gives considerable information, not merely about the character of its curvature, but (as we shall see) also about other geometric invariants, notably null geodesics. |
 | | In particular, for type D spacetimes such as Kerr's, these congruences are not only geodesic but also "shearfree"--roughly speaking, if a beam of such light initially has circular cross-section, then it keeps this property as it propagates. |
 | | A final perspective on Kerr spacetime is provided by the Goldberg-Sachs theorem, which for arbitrary Ricci-flat spacetimes gives necessary and sufficient curvature conditions for the existence of shear-free geodesic null congruences. |
| www.math.ucla.edu /~bon/kerr/intro5.html (336 words) |
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