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Hawking emission of gravitons in higher dimensions: non-rotating black holes

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arxiv hep-th/0512116 v3 pith:MCIGJEWH submitted 2005-12-09 hep-th gr-qchep-ph

Vitor Cardoso , Marco Cavaglia , Leonardo Gualtieri This is my paper · ORCID
classification hep-thgr-qchep-ph
keywords blackgravitonsdimensionsemissionholesmodelnon-rotatingabsorption
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We compute the absorption cross section and the total power carried by gravitons in the evaporation process of a higher-dimensional non-rotating black hole. These results are applied to a model of extra dimensions with standard model fields propagating on a brane. The emission of gravitons in the bulk is highly enhanced as the spacetime dimensionality increases. The implications for the detection of black holes in particle colliders and ultrahigh-energy cosmic ray air showers are briefly discussed.

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  1. Micro Black Hole Dark Matter

    hep-th 2025-06 conditional novelty 5.0 of 10

    Micro black holes could survive as dark matter down to 10^{-5} Planck masses if extra dimensions or many species strengthen the memory-burden suppression of their evaporation.

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