GEOMETRIC CHARACTERIZATIONS OF THE KERR ISOLATED HORIZON

DOI10.1142/S0218271802001986zbMath1062.83528arXivgr-qc/0101008WikidataQ58879846 ScholiaQ58879846MaRDI QIDQ4674729

Tomasz Pawlowski, Jerzy Lewandowski

Publication date: 18 May 2005

Published in: International Journal of Modern Physics D (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/gr-qc/0101008

Mathematics Subject Classification ID

Black holes (83C57) Applications of differential geometry to physics (53Z05)

Related Items

Analytic continuation of the rotating black hole state counting, Kerr isolated horizons in Ashtekar and Ashtekar-Barbero connection variables, The Petrov type D equation on genus \(>0\) sections of isolated horizons, Non-singular Kerr-NUT-de Sitter spacetimes, Isolated and dynamical horizons and their applications, Modelling black holes with angular momentum in loop quantum gravity, The Petrov type D isolated null surfaces, Past horizons in twisting algebraically special space–times

Cites Work

• On further generalization of the rigidity theorem for spacetimes with a stationary event horizon or a compact Cauchy horizon
• Generic Isolated Horizons and Their Applications