Is there a definition of a black hole in a generic spacetime? In some books, for example Wald's, black holes are defined for asymptotically flat spacetime with strong asymptotic predictability, although the definition makes sense without the second condition. Is there a notion of a black hole in general spacetime, not necessarily asymptotically flat? Or is it the case that there is not a "natural" or agreed upon definition?
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\mathscr{I}enclosed in dollar signs. In the most generality there is no definition I am aware of. But you can (probably) define it for asymptotically AdS/hyperbolic space-times and space-times admitting some sort of conformal compactification, modulo some technical issues on decay rates of the metric. – Willie Wong Oct 18 '11 at 21:32