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Can Centauros or Chirons be the first observations of evaporating mini black holes?

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arxiv hep-ph/0311318 v2 pith:3QQLVPN5 submitted 2003-11-25 hep-ph

A. Mironov , A. Morozov , T.N. Tomaras This is my paper
classification hep-ph
keywords blackholesminiargueatmospherecentaurocentauroscharacteristics
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We argue that the signals expected from the evaporation of mini black holes - predicted in TeV-scale gravity models with large extra dimensions, and possibly produced in ultra high energy collisions in the atmosphere - are quite similar to the characteristics of the Centauro events, an old mystery of cosmic-ray physics.

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Cited by 1 Pith paper

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  1. Relativistic strange quark stars in Lovelock gravity

    gr-qc 2019-07 unverdicted novelty 5.0 of 10

    Numerical computation of mass-radius profiles, compactness, and gravitational redshift for strange quark stars in 5D Gauss-Bonnet gravity across several values of the Gauss-Bonnet parameter.

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