2012
DOI: 10.1088/0264-9381/30/1/013001
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Algebraic classification of higher dimensional spacetimes based on null alignment

Abstract: We review recent developments and applications of the classification of the Weyl tensor in higher dimensional Lorentzian geometries. First, we discuss the general setup, i.e. main definitions and methods for the classification, some refinements and the generalized Newman-Penrose and Geroch-Held-Penrose formalisms. Next, we summarize general results, such as a partial extension of the Goldberg-Sachs theorem, characterization of spacetimes with vanishing (or constant) curvature invariants and the peeling behavio… Show more

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Cited by 116 publications
(305 citation statements)
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References 186 publications
(903 reference statements)
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“…In addition to (6), the remaining Ricci rotation coefficients are defined by (see [21] and references therein)…”
Section: A Definitions Of the Ricci Rotation Coefficientsmentioning
confidence: 99%
“…In addition to (6), the remaining Ricci rotation coefficients are defined by (see [21] and references therein)…”
Section: A Definitions Of the Ricci Rotation Coefficientsmentioning
confidence: 99%
“…The Weyl tensor of type-N spacetimes have been studied in detail in [12][13][14][15]. Let ℓ, n and m (i) , (i = 2, · · · D − 1) be a null tetrad frame with…”
Section: Type-n Weyl and Traceless Ricci Tensorsmentioning
confidence: 99%
“…As an application of our result, we show that any type-N Einstein space R µν = R D g µν solve the field equations of the Lanczos-Lovelock theory. In addition, for a special choice of the parameters, any spacetime metric having type-N Weyl and traceless Ricci tensors with constant Ricci scalar solve the specific Lanczos-Lovelock theory.To find exact asymptotically AdS solutions of a generic higher derivative theory, we shall make use of general results of [12][13][14][15][16] which utilize the boost weight formalism.Type-N Weyl and Traceless Ricci tensors The Weyl tensor of type-N spacetimes have been studied in detail in [12][13][14][15]. Let ℓ, n and m (i) , (i = 2, · · · D − 1) be a null tetrad frame with…”
mentioning
confidence: 99%
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“…Most of the activity on the subject has been focused on asymptotically flat models, the solutions of GR without a cosmological constant. From 1980s, exact gravitational waves have been studied also in GR with a cosmological constant (GR Λ ) [5][6][7], see also [8]; for higher-dimensional extensions, see [9][10][11][12][13]. In particular, exact gravitational waves with an AdS asymptotic behavior attracted a lot of interest in regard to the AdS/CFT correspondence [14,15].…”
Section: Introductionmentioning
confidence: 99%