2000
DOI: 10.1088/0264-9381/17/22/314
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A class of conformally Einstein metrics

Abstract: A class of spacetime metrics with coefficients depending on a single null coordinate is introduced. The equation of the null cone at an arbitrary point is obtained in explicit form. It is shown that every metric in this class has a Weyl tensor of Petrov type N and is conformal to a metric satisfying the Einstein vacuum equations. The metrics belonging to a particular subclass are shown to be conformal to certain plane-wave solutions in general relativity. The properties of a generalization of these metrics to … Show more

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Cited by 4 publications
(4 citation statements)
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“…As of the time of writing, the author has been able to show by direct calculation that the prototypical space-times of Kapadia & Sparling (2000) are coherent, at least for complex homogeneous input functions, giving the first known example of a curved space-time that is such. Note that this proposed classification is inherently non-perturbative and potentially gives a coordinateindependent definition of dynamical chaos (Cvitanović et al 2004).…”
Section: The X-transformmentioning
confidence: 99%
“…As of the time of writing, the author has been able to show by direct calculation that the prototypical space-times of Kapadia & Sparling (2000) are coherent, at least for complex homogeneous input functions, giving the first known example of a curved space-time that is such. Note that this proposed classification is inherently non-perturbative and potentially gives a coordinateindependent definition of dynamical chaos (Cvitanović et al 2004).…”
Section: The X-transformmentioning
confidence: 99%
“…Riemannian manifolds (M, g) for which there exists a pointwise conformal deformation g = e 2u g, u ∈ C ∞ (M ), such that the new metric g is Einstein. This problem has received a considerable amount of attention by mathematicians and physicists in the last decades: just to mention some old and recent papers we cite the pioneering work of Brinkmann, [4], Yano and Nagano, [35], Gover and Nurowski, [17], Kapadia and Sparling, [21], Derdzisnki and Maschler, [15], and references therein. In particular in [17] the authors describe two necessary integrability conditions for the existence of the conformal deformation g realizing the Einstein metric.…”
Section: Introductionmentioning
confidence: 99%
“…There is only one non-conformally flat case where the relevant calculations have been carried out in detail, that of the Kapadia [15] metric:…”
Section: Introductionmentioning
confidence: 99%