Tunneling from the past horizon

Subeom Kang and Dong-han Yeom
Phys. Rev. D 97, 086011 – Published 19 April 2018

Abstract

We investigate a tunneling and emission process of a thin-shell from a Schwarzschild black hole, where the shell was initially located beyond the Einstein-Rosen bridge and finally appears at the right side of the Penrose diagram. In order to obtain such a solution, we should assume that the areal radius of the black hole horizon increases after the tunneling. Hence, there is a parameter range such that the tunneling rate is exponentially enhanced, rather than suppressed. We may have two interpretations regarding this. First, such a tunneling process from the past horizon is improbable by physical reasons; second, such a tunneling is possible in principle, but in order to obtain a stable Einstein-Rosen bridge, one needs to restrict the parameter spaces. If such a process is allowed, this can be a nonperturbative contribution to Einstein-Rosen bridges as well as eternal black holes.

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  • Received 12 December 2017

DOI:https://doi.org/10.1103/PhysRevD.97.086011

© 2018 American Physical Society

Physics Subject Headings (PhySH)

Gravitation, Cosmology & Astrophysics

Authors & Affiliations

Subeom Kang1,2,* and Dong-han Yeom3,4,†

  • 1Department of Physics, KAIST, Daejeon 34141, Republic of Korea
  • 2Center for Theoretical Physics of the Universe, Institute for Basic Science (IBS), Daejeon 34051, Republic of Korea
  • 3Asia Pacific Center for Theoretical Physics, Pohang 37673, Republic of Korea
  • 4Department of Physics, POSTECH, Pohang 37673, Republic of Korea

  • *ksb527@kaist.ac.kr
  • innocent.yeom@gmail.com

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Issue

Vol. 97, Iss. 8 — 15 April 2018

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