Advanced Search

Query:

Fill in the form and click »Search«...

Format:

Display: entries per page entries

Zbl 1161.83003
Duggal, K.L.
Time-dependent black hole horizons on spacetime solutions of Einstein's equations with initial data. (English)
[A] Plaue, M. (ed.) et al., Advances in Lorentzian geometry. Aachen: Shaker Verlag. 51-61 (2008). ISBN 978-3-8322-7786-4/pbk

For non-static black holes, the author presents a method how to define a horizon, called a dynamical horizon. To this end he introduces the notion of a FOTH, a future outer trapped horizon. Methods applied cover: foliations of space-time into space-like hypersurfaces, which in a certain limit degenerate to a foliation into null hypersurfaces; the use of conformal Killing vectors; comparison between geometrically and physically motivated conditions. Finally, black hole uniqueness conditions are mentioned.
[Hans-Jürgen Schmidt (Potsdam)]

MSC 2000:: *83C05 Einstein's equations
83C57 Black holes
53C50 Lorentz manifolds, manifolds with indefinite metrics
83C75 Space-time singularities, etc.

Keywords: dynamical horizon

Comment on this Item PDF MathML XML ASCII DVI PS BibTeX Online Ordering Article

	Scientific prize winners of the ICM 2010
	Overhang
	Lie groups, physics and geometry. An introduction for physicists, engineers and chemists.

Advanced Search

Zentralblatt MATH Berlin [Germany]