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Bounds on large extra dimensions from the simulation of black hole events at the LHC

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arxiv 1507.01632 v1 pith:6JPMQYHD submitted 2015-07-06 hep-ph hep-exhep-th

classification hep-phhep-exhep-th
keywords blackholeformationholesscaleboundsdimensionsextra
verification ladder T0 review T1 audit T2 compute T3 formal
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abstract

If large extra dimensions exist, the Planck scale may be as low as a TeV and microscopic black holes may be produced in high-energy particle collisions at this energy scale. We simulate microscopic black hole formation at the Large Hadron Collider and compare the simulation results with recent experimental data by the Compact Muon Solenoid collaboration. The absence of observed black hole events in the experimental data allows us to set lower bounds on the Planck scale and various parameters related to microscopic black hole formation for a number ($3-6$) of extra dimensions. Our analysis sets lower bounds on the fundamental Planck scale ranging from 0.6 TeV to 4.8 TeV for black holes fully decaying into Standard Model particles and 0.3 TeV to 2.8 TeV for black holes settling down to a remnant, depending on the minimum allowed black hole mass at formation. Formation of black holes with mass less than 5.2 TeV to 6.5 TeV (SM decay) and 2.2 TeV to 3.4 TeV (remnant) is excluded at 95\% C.L. Our analysis shows consistency with and difference from the CMS results.

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Cited by 1 Pith paper

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Initial data for a black string and a Kaluza-Klein bubble: Space-dependent compactification radius

    gr-qc 2025-01 conditional novelty 6.0 of 10

    New analytic and numerical initial data are constructed for Kaluza-Klein spacetimes with a space-dependent compactification radius, covering black strings, naked or hidden KK bubbles, and multiple black strings.

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