WANDs of the Black Ring
arXiv:gr-qc/0501003 · doi:10.1007/s10714-005-0110-3
Abstract
Necessary conditions for various algebraic types of the Weyl tensor are determined. These conditions are then used to find Weyl aligned null directions for the black ring solution. It is shown that the black ring solution is algebraically special, of type I_i, while locally on the horizon the type is II. One exceptional subclass - the Myers-Perry solution - is of type D.
9 pages, 3 figures
References in corpus (2)
Cited by in corpus (38)
- Black Holes in Higher Dimensions
- Classification of the Weyl Tensor in Higher Dimensions and Applications
- Algebraic classification of higher dimensional spacetimes based on null alignment
- Robinson-Trautman spacetimes in higher dimensions
- Generalization of the Geroch-Held-Penrose formalism to higher dimensions
- Type D Einstein spacetimes in higher dimensions
- Minimal tensors and purely electric or magnetic spacetimes of arbitrary dimension
- Higher dimensional Kerr-Schild spacetimes
- Weyl doubling
- Superradiant instability of large radius doubly spinning black rings
- On a five-dimensional version of the Goldberg-Sachs theorem
- Identification of black hole horizons using scalar curvature invariants
- Bel-Debever criteria for the classification of the Weyl tensors in higher dimensions
- Scalar Polynomial Curvature Invariant Vanishing on the Event Horizon of Any Black Hole Metric Conformal to a Static Spherical Metric
- Classification of Higher Dimensional Spacetimes
- Spinor-helicity and the algebraic classification of higher-dimensional spacetimes
- An Extended Kerr-Schild Ansatz
- Spinor classification of the Weyl tensor in five dimensions
- Black rings with a small electric charge: gyromagnetic ratios and algebraic alignment
- On higher dimensional Einstein spacetimes with a warped extra dimension
- Charging Kerr-Schild spacetimes in higher dimensions
- Extended Kerr-Schild spacetimes: General properties and some explicit examples
- The Cartan Algorithm in Five Dimensions
- Refinements of the Weyl tensor classification in five dimensions
- Optical structures, algebraically special spacetimes, and the Goldberg-Sachs theorem in five dimensions
- Universal Black Holes
- On the Goldberg-Sachs theorem in higher dimensions in the non-twisting case
- Surface Geometry of 5D Black Holes and Black Rings
- Curvature invariant characterization of event horizons of four-dimensional black holes conformal to stationary black holes
- Algebraic classification of five-dimensional spacetimes using scalar invariants
- Horizon Detection and Higher Dimensional Black Rings
- Algebraic classification of the Weyl tensor in higher dimensions based on its "superenergy" tensor
- On the Weyl Tensor Classification in All Dimensions and its Relation with Integrability Properties
- Nonvanishing Local Scalar Invariants even in VSI Spacetimes with all Polynomial Curvature Scalar Invariants Vanishing
- On the algebraic classification of spacetimes
- Generalized wave operators, weighted Killing fields, and perturbations of higher dimensional spacetimes
- Ultrarelativistic boost of spinning black rings
- On the uniqueness of the Kerr-(A)dS metric as a type II(D) solution in six dimensions