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Stationary Black Holes: Uniqueness and Beyond

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dc.creator Heusler Markus
dc.date 1998
dc.date.accessioned 2013-06-01T11:42:50Z
dc.date.available 2013-06-01T11:42:50Z
dc.date.issued 2013-06-01
dc.identifier http://www.livingreviews.org/lrr-1998-6
dc.identifier http://www.doaj.org/doaj?func=openurl&genre=article&issn=14338351&date=1998&volume=1&issue=&spage=6
dc.identifier.uri http://koha.mediu.edu.my:8181/jspui/handle/123456789/8633
dc.description The spectrum of known black hole solutions to the stationary Einstein equations has increased in an unexpected way during the last decade. In particular, it has turned out that not all black hole equilibrium configurations are characterized by their mass, angular momentum and global charges. Moreover, the high degree of symmetry displayed by vacuum and electro-vacuum black hole space-times ceases to exist in self-gravitating non-linear field theories. This text aims to review some of the recent developments and to discuss them in the light of the uniqueness theorem for the Einstein-Maxwell system.
dc.publisher Albert Einstein Institut, Max-Planck Institute for Gravitati
dc.source Living Reviews in Relativity
dc.subject Mathematical Relativity
dc.title Stationary Black Holes: Uniqueness and Beyond


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