Trapping Black Hole Remnants
Sabine Hossenfelder (Univ. of Arizona), Benjamin Koch (FIGSS, U, Frankfurt), Marcus Bleicher (U Frankfurt)

TL;DR
This paper explores the possibility of trapping charged black hole remnants produced at the LHC, which could enable detailed study of their evaporation process and provide insights into quantum gravity effects.
Contribution
It proposes a method to trap charged black hole remnants from TeV-scale black holes, facilitating precise investigation of their late-stage evaporation characteristics.
Findings
Charged black hole remnants can be trapped for detailed study.
Trapped remnants offer a background-free environment for evaporation analysis.
Potential to extract information about quantum gravity effects from remnants.
Abstract
Large extra dimensions lower the Planck scale to values soon accessible. The production of TeV mass black holes at the {\sc LHC} is one of the most exciting predictions. However, the final phases of the black hole's evaporation are still unknown and there are strong indications that a black hole remnant can be left. Since a certain fraction of such objects would be electrically charged, we argue that they can be trapped. In this paper, we examine the occurrence of such charged black hole remnants. These trapped remnants are of high interest, as they could be used to closely investigate the evaporation characteristics. Due to the absence of background from the collision region and the controlled initial state, the signal would be very clear. This would allow to extract information about the late stages of the evaporation process with high precision.
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Taxonomy
TopicsBlack Holes and Theoretical Physics · Particle physics theoretical and experimental studies · Cosmology and Gravitation Theories
