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100 Years of Relativity Space-Time Structure: Einstein and Beyond ...

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118 P. T. ChruścielBecause <strong>of</strong> the high symmetry, one expects that “all black holes willeventually merge”, so that the event horizon will be a connected hypersurfacein space-time.5.3. Black holes <strong>and</strong> gluing methodsA recent alternate technique for gluing initial data sets is given in Refs. 59.In this approach, general initial data sets on compact manifolds or withasymptotically Euclidean or hyperboloidal ends are glued together to producesolutions <strong>of</strong> the constraint equations on the connected sum manifolds.Only very mild restrictions on the original initial data are needed. The neckregions produced by this construction are again <strong>of</strong> Schwarzschild type. Theoverall strategy <strong>of</strong> the construction is similar to that used in many previousgluing constructions in geometry. Namely, one takes a family <strong>of</strong> approximatesolutions to the constraint equations <strong>and</strong> then attempts to perturbthe members <strong>of</strong> this family to exact solutions. There is a parameter η whichmeasures the size <strong>of</strong> the neck, or gluing region; the main difficulty is causedby the tension between the competing dem<strong>and</strong>s that the approximate solutionsbecome more nearly exact as η → 0 while the underlying geometry <strong>and</strong>analysis become more singular. In this approach, the conformal method <strong>of</strong>solving the constraints is used, <strong>and</strong> the solution involves a conformal factorwhich is exponentially close to one (as a function <strong>of</strong> η) away from the neckregion. It has been shown 30 that the deformation can actually be localisednear the neck in generic situations.Consider, now, an asymptotically flat time-symmetric initial data set,to which several other time-symmetric initial data sets have been glued bythis method. If the gluing regions are made small enough, the existence<strong>of</strong> a non-trivial minimal surface, hence <strong>of</strong> an apparent horizon, follows byst<strong>and</strong>ard results. This implies the existence <strong>of</strong> a black hole region in themaximal globally hyperbolic development <strong>of</strong> the data.It is shown in Ref. 32 that the intersection <strong>of</strong> the event horizon with theinitial data hypersurface will have more than one connected component forseveral families <strong>of</strong> glued initial data sets.AcknowledgementsThe author is grateful to Robert Beig for many useful discussions, to KayllLake for comments <strong>and</strong> electronic figures, <strong>and</strong> to Jean-Philippe Nicolasfor figures. The presentation here borrows heavily on Ref. 7, <strong>and</strong> can bethought <strong>of</strong> as an extended version <strong>of</strong> that work.

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