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arXiv · 0912.2028

Black hole gas in TeV-gravity models

Monica Borunda·Manuel Masip
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Abstract

In a plasma at temperature close to the fundamental scale a small fraction of particles will experience transplanckian collisions that may result in microscopic black holes (BHs). We study the dynamics of a system (a black hole gas) defined by radiation at a given temperature coupled to a distribution of BHs of different mass. Our analysis includes the production of BHs in photon-photon collisions, BH evaporation, the absorption of radiation, collisions of two BHs to give a larger one, and the effects of the expansion. We find that the system may follow two different generic paths depending on the initial temperature of the plasma.

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Monica Borunda, Manuel Masip. 2009-12-10. Black hole gas in TeV-gravity models. https://doi.org/10.1088/1742-6596%2F229%2F1%2F012023

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