Holographic Entropy Packing inside a Black Hole

Aharon Davidson and Ilya Gurwich
Phys. Rev. Lett. 106, 151301 – Published 11 April 2011

Abstract

If general relativity is spontaneously induced, the black hole limit is governed by a phase transition which occurs precisely at the would-have-been horizon. The exterior Schwarzschild solution then connects with a novel core of vanishing spatial volume. The Kruskal structure, admitting the exact Hawking imaginary time periodicity, is recovered, with the conic defect defused at the origin, rather than at the horizon. The entropy stored inside any interior sphere is universal, equal to a quarter of its surface area, thus locally saturating the ’t Hooft–Susskind holographic bound. The associated Komar mass and material energy functions are nonsingular.

  • Received 12 August 2010

DOI:https://doi.org/10.1103/PhysRevLett.106.151301

© 2011 American Physical Society

Authors & Affiliations

Aharon Davidson* and Ilya Gurwich

  • Physics Department, Ben-Gurion University of the Negev, Beer-Sheva 84105, Israel

  • *davidson@bgu.ac.il
  • gurwichphys@gmail.com

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Issue

Vol. 106, Iss. 15 — 15 April 2011

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