A local non-negative initial data scalar characterisation of the Kerr solution
arXiv:1510.07561 · doi:10.1103/PhysRevD.92.124053
Abstract
For any vacuum initial data set, we define a local, non-negative scalar quantity which vanishes at every point of the data hypersurface if and only if the data are {\em Kerr initial} data. Our scalar quantity only depends on the quantities used to construct the vacuum initial data set which are the Riemannian metric defined on the initial data hypersurface and a symmetric tensor which plays the role of the second fundamental form of the embedded initial data hypersurface. The dependency is {\em algorithmic} in the sense that given the initial data one can compute the scalar quantity by algebraic and differential manipulations, being thus suitable for an implementation in a numerical code. The scalar could also be useful in studies of the non-linear stability of the Kerr solution because it serves to measure the deviation of a vacuum initial data set from the Kerr initial data in a local and algorithmic way.
18 pages, no figures. Typos corrected and dropped artificial restriction on the vacuum initial data set used to define the positive scalar. To appear in Physical Review D
References in corpus (6)
- The Kerr Metric
- Dynamical laws of superenergy in General Relativity
- An intrinsic characterization of the Kerr metric
- On the construction of a geometric invariant measuring the deviation from Kerr data
- The "non-Kerrness" of domains of outer communication of black holes and exteriors of stars
- A set of invariant quality factors measuring the deviation from the Kerr metric
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