English

A local non-negative initial data scalar characterisation of the Kerr solution

General Relativity and Quantum Cosmology 2015-12-30 v2

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.

Cite

@article{arxiv.1510.07561,
  title  = {A local non-negative initial data scalar characterisation of the Kerr solution},
  author = {Alfonso García-Parrado Gómez-Lobo},
  journal= {arXiv preprint arXiv:1510.07561},
  year   = {2015}
}

Comments

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

R2 v1 2026-06-22T11:29:09.174Z