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Gauss-bonnet black holes and possibilities for their experimental search

  • Nuclei, Particles, Fields, Gravitation, and Astrophysics
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Abstract

Corollaries of gravity models with second-order curvature corrections in the form of a Gauss-Bonnet term and possibilities (or impossibilities) for their experimental search or observations are discussed. The full version of the four-dimensional Schwarzschild-Gauss-Bonnet black hole solution and the constraint on the possible minimal black hole mass following from this model are considered. Using our solution as a model for the final stages of Hawking evaporation of black holes with a low initial mass (up to 1015 g) whose lifetime is comparable to that of our Universe, we have revealed differences in the patterns of evaporation: we have obtained high values of the emitted energy and showed the impossibility of an experimental search for primordial black holes by their evaporation products. Scenarios for the evaporation of Gauss-Bonnet black holes in multidimensional gravity models and possibilities for their experimental search are also discussed.

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  1. Sternberg Astronomical Institute, Universitetskii pr. 13, Moscow, 119992, Russia

    S. O. Alexeyev & K. A. Rannu

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  1. S. O. Alexeyev
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  2. K. A. Rannu
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Correspondence to S. O. Alexeyev.

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Original Russian Text © S.O. Alexeyev, K.A. Rannu, 2012, published in Zhurnal Eksperimental’noi i Teoreticheskoi Fiziki, 2012, Vol. 141, No. 3, pp. 463–487.

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Alexeyev, S.O., Rannu, K.A. Gauss-bonnet black holes and possibilities for their experimental search. J. Exp. Theor. Phys. 114, 406–427 (2012). https://doi.org/10.1134/S1063776112030119

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