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Dynamical formation of black holes due to the condensation of matter field

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arxiv 1105.5898 v1 pith:J6UPGTXK submitted 2011-05-30 math.AP gr-qc

classification math.APgr-qc
keywords fieldformationtrappedblackcondensationcoupledelectromagnetichand
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The purpose of the paper is to understand a mechanism of evolutionary formation of trapped surfaces when there is an electromagnetic field coupled to the background space-time. Based on the short pulse ansatz, on a given finite outgoing null hypersurface which is free of trapped surfaces, we exhibit an open set of initial data for Einstein equations coupled with a Maxwell field, so that a trapped surface forms along the Einstein-Maxwell flow. On one hand, this generalizes the black-hole-formation results of Christodoulou and Klainerman-Rodnianski. In fact, by switching off the electromagnetic field in our main theorem, we can retrieve their results in vacuum. On the other hand, this shows that the formation of black hole can be purely due to the condensation of Maxwell field on the initial null hypersurface where there is no incoming gravitational energy.

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Cited by 3 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Formation of multiple Black Holes from Cauchy data

    gr-qc 2025-06 conditional novelty 8.0 of 10

    The authors construct smooth vacuum initial data without trapped surfaces whose future evolution produces N causally independent trapped surfaces.

  2. Formation of trapped surfaces for the Einstein--Maxwell--charged scalar field system

    math.AP 2025-04 conditional novelty 8.0 of 10

    A scale-critical, symmetry-free trapped surface formation theorem for the Einstein-Maxwell-charged scalar field system, including a dynamic charging process along past null infinity.

  3. On Kerr black hole formation with complete apparent horizon and a new approach toward Penrose inequality

    gr-qc 2025-05 conditional novelty 7.0 of 10

    The authors prove that scale-critical short-pulse initial data can produce global Kerr black hole formation spacetimes with a complete apparent horizon, and they derive dynamical and spacetime Penrose inequalities in ...

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