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Black hole Meissner effect and entanglement

Robert F. Penna*

  • Department of Physics and Kavli Institute for Astrophysics and Space Research, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA

  • *rpenna@mit.edu
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Phys. Rev. D 90, 043003 – Published 4 August, 2014

DOI: https://doi.org/10.1103/PhysRevD.90.043003

Abstract

Extremal black holes tend to expel magnetic and electric fields. Fields are unable to reach the horizon because the length of the black hole throat blows up in the extremal limit. The length of the throat is related to the amount of entanglement between modes on either side of the horizon. So it is natural to try to relate the black hole Meissner effect to entanglement. We derive the black hole Meissner effect directly from the low temperature limit of two-point functions in the Hartle-Hawking vacuum. Then we discuss several new examples of the black hole Meissner effect, its applications to astrophysics, and its relationship to gauge invariance.

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Phys. Rev. D 90, 043003– Published 4 August, 2014
  • Received 16 June 2014

© 2014 American Physical Society

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