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Black hole formation by incoming electromagnetic radiation

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arxiv 1408.2778 v2 pith:5JWBEE36 submitted 2014-08-12 gr-qc hep-th

José M. M. Senovilla This is my paper · ORCID
classification gr-qchep-th
keywords blackelectromagneticformationholesradiationsolutioncollapsecondition
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I revisit a known solution of the Einstein field equations to show that it describes the formation of non-spherical black holes by the collapse of pure electromagnetic monochromatic radiation. Both positive and negative masses are feasible without ever violating the dominant energy condition. The solution can also be used to model the destruction of naked singularities and the evaporation of white holes by emission or reception of light.

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  1. Toroidal black holes in four dimensions

    gr-qc 2025-04 conditional novelty 7.0 of 10

    An explicit, singularity-free exterior for a four-dimensional toroidal black hole is constructed by gluing a locally vacuum Rindler tube to Minkowski space through an interpolating matter region, with energy condition...

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