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Black hole Meissner effect and entanglement

Author(s)
Penna, Robert
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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.
Date issued
2014-08
URI
http://hdl.handle.net/1721.1/88671
Department
Massachusetts Institute of Technology. Department of Physics; MIT Kavli Institute for Astrophysics and Space Research
Journal
Physical Review D
Publisher
American Physical Society
Citation
Penna, Robert F. "Black hole Meissner effect and entanglement." Phys. Rev. D 90, 043003 (August 2014). © 2014 American Physical Society
Version: Final published version
ISSN
1550-7998
1550-2368

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