Outermost apparent horizon conjecture for black holes

Let

beinitialdataasinTheorem1,withmaximalfuturedevelopment,quotientspacetimebe initial data as in Theorem 1, with maximal future development, quotient spacetime

, black-hole region, apparent horizon

,andoutermostapparenthorizon, and outermost apparent horizon

. Assume the black hole is sub-extremal in the limit and

.Outermostapparenthorizonconjecture.Thereanonemptyasymptoticallyconnectedcomponent. **Outermost apparent horizon conjecture.** There \exists a nonempty asymptotically connected component

of the outermost apparent horizon that terminates at i+i^+. Moreover, in a sufficiently small neighborhood

of $i^+$,

\mathcal{A}'\cap\mathcal{U}=\mathcal{A}\cap\mathcal{U},

andand

I^+(\mathcal{A}\cap\mathcal{U})\cap\mathcal{Q}^+\subset\mathcal{T}.

The conjecture describes the geometry of the trapped region near $i^+$ and, according to the paper, would imply continuous extension of $r$ to

near i+i^+. It remains unresolved in the supplied source.

Sources & referencesView supporting material

Primary source

Jonathan Kommemi, “The global structure of spherically symmetric charged scalar field spacetimes”, arXiv:1107.0949 (2013).

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