Algebraic classification of Robinson-Trautman spacetimes

Abstract

We consider a general class of four-dimensional geometries admitting a null vector field that has no twist and no shear but has an arbitrary expansion. We explicitly present the Petrov classification of such Robinson-Trautman (and Kundt) gravitational fields, based on the algebraic properties of the Weyl tensor. In particular, we determine all algebraically special subcases when the optically privileged null vector field is a multiple principal null direction (PND), as well as all the cases when it remains a single PND. No field equations are a priori applied, so that our classification scheme can be used in any metric theory of gravity in four dimensions. In the classic Einstein theory this reproduces previous results for vacuum spacetimes, possibly with a cosmological constant, pure radiation and electromagnetic field, but can be applied to an arbitrary matter content. As non-trivial explicit examples we investigate specific algebraic properties of the Robinson-Trautman spacetimes with a free scalar field, and also black hole spacetimes in the pure Einstein-Weyl gravity.

23 pages, no figures, slightly extended version of the Phys. Rev. D paper

References in corpus (7)

• Black Holes in Higher-Derivative Gravity
• Robinson-Trautman spacetimes in higher dimensions
• Algebraic classification of higher dimensional spacetimes based on null alignment
• Robinson-Trautman spacetimes with an electromagnetic field in higher dimensions
• Static and radiating p-form black holes in the higher dimensional Robinson-Trautman class
• Refinements of the Weyl tensor classification in five dimensions
• Algebraic structure of Robinson-Trautman and Kundt geometries in arbitrary dimension

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• Robinson-Trautman solutions with scalar hair and Ricci flow
• Supersymmetry of the Robinson-Trautman solution
• Wedging spacetime principal null directions
• Local and Approximate classification of spacetimes in the transverse frames