Black Holes at the Large Hadron Collider

Savas Dimopoulos and Greg Landsberg
Phys. Rev. Lett. 87, 161602 – Published 27 September 2001
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Abstract

If the scale of quantum gravity is near TeV, the CERN Large Hadron Collider will be producing one black hole (BH) about every second. The decays of the BHs into the final states with prompt, hard photons, electrons, or muons provide a clean signature with low background. The correlation between the BH mass and its temperature, deduced from the energy spectrum of the decay products, can test Hawking’s evaporation law and determine the number of large new dimensions and the scale of quantum gravity.

  • Received 28 June 2001

DOI:https://doi.org/10.1103/PhysRevLett.87.161602

©2001 American Physical Society

Authors & Affiliations

Savas Dimopoulos1 and Greg Landsberg2

  • 1Physics Department, Stanford University, Stanford, California 94305-4060
  • 2Department of Physics, Brown University, Providence, Rhode Island 02912

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Vol. 87, Iss. 16 — 15 October 2001

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