Non-existence of short hairs for static black holes

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dc.contributor.author Acharya, Soham
dc.contributor.author Sarkar, Sudipta
dc.coverage.spatial United States of America
dc.date.accessioned 2024-02-23T07:55:05Z
dc.date.available 2024-02-23T07:55:05Z
dc.date.issued 2024-02
dc.identifier.citation Acharya, Soham and Sarkar, Sudipta, "Non-existence of short hairs for static black holes", arXiv, Cornell University Library, DOI: arXiv:2402.09044, Feb. 2024.
dc.identifier.issn 2331-8422
dc.identifier.uri https://doi.org/10.48550/arXiv.2402.09044
dc.identifier.uri https://repository.iitgn.ac.in/handle/123456789/9794
dc.description.abstract The black hole no-short hair theorem establishes a universal lower bound on the extension of hairs outside any 4-dimensional spherically symmetric black hole solutions. We generalise this theorem beyond spherical symmetry, specifically for static, axisymmetric hairy black hole solutions and prove that the ``hairosphere'' must extend beyond the radial extent of the innermost light ring.
dc.description.statementofresponsibility by Soham Acharya and Sudipta Sarkar
dc.language.iso en_US
dc.publisher Cornell University Library
dc.title Non-existence of short hairs for static black holes
dc.type Article
dc.relation.journal arXiv


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