Hawking Radiation around the Wormhole Sung-Won Kim (Ewha Womans - - PowerPoint PPT Presentation

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Hawking Radiation around the Wormhole Sung-Won Kim (Ewha Womans - - PowerPoint PPT Presentation

Hawking Radiation around the Wormhole Sung-Won Kim (Ewha Womans University) In collaboration with S. Hayward APS2012 - Yukawa 1 Contents Motivation Surface Gravity Wormhole Temperature Hamilton-Jacobi Equation Summary


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Hawking Radiation around the Wormhole

Sung-Won Kim (Ewha Womans University)

In collaboration with S. Hayward

1 APS2012 - Yukawa

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Contents

  • Motivation
  • Surface Gravity
  • Wormhole Temperature
  • Hamilton-Jacobi Equation
  • Summary

2 APS2012 - Yukawa

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Motivation

  • Recent active researches on dynamical horizon
  • Morris-Thorne wormhole throat is a double

trapping horizon

  • Potential form around the throat is similar to

that of event horizon

  • Temperature of wormhole issue is revisited

3 APS2012 - Yukawa

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Surface Gravity

  • Several Definitions

– Killing vector definition (Wald) – Acceleration (Abreu & Visser) – 2D Expansion (Jacobson & Parentani) – Minimality condition (Hayward)

  • Recent review (Nielson & Yoon; Pielahn, Kunstatter, &

Nielson)

4 APS2012 - Yukawa

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Wormhole temperature

  • By Killing vector definition (Hong & Kim, 2006)
  • Negative temperature

with exotic matter

APS2012 - Yukawa 5

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Trapping Horizon

  • A sphere of radius r=(A/4π)1/2 is

– Untrapped for spatial g-1(dr ) – Marginal for null g-1(dr ) – Trapped for temporal g-1(dr )

  • Trapping horizon: A hypersurface foliated by

marginal spheres

6 APS2012 - Yukawa

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Surface gravity at trapping horizon (Hayward, 1998)

  • Kodama vector: preferred flow of time
  • Normal to sphere of symmetry
  • Surface gravity
  • Spherically symmetric metric

APS2012 - Yukawa 7

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Wormhole Case

8 APS2012 - Yukawa

  • Morris-Thorne wormhole:
  • Regge-Wheeler tortoise coordinate form
  • Surface gravity
  • By Einstein’s equation (2m≠8πr 3τ )
  • Flare-out condition
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Hamilton-Jacobi equation (1/3)

  • With redefinition of v =t*+r* as

dt =C1/2dt*, dr = eφCdr*, C =1-2m/r

  • Advanced Eddington-Finkelstein form (φ =Ψ)
  • WKB approximation of the tunneling probability Г

is the imaginary part of action I

9 APS2012 - Yukawa

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Hamilton-Jacobi equation (2/3)

  • In thermal form
  • Action
  • Energy and momentum
  • Hamilton-Jacobi equation
  • r
  • Solution for outgoing mode
  • I has a pole

APS2012 - Yukawa 10

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Hamilton-Jacobi equation (3/3)

  • For the case of (2m=8πr 3τ )
  • The imaginary part of the action
  • By comparing with the thermal form

APS2012 - Yukawa 11

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Summary

  • Various definitions of the surface gravity
  • Wormhole’s Hawking temperature
  • Checking by Hamilton-Jacobi tunneling method, we

can consider the Hawking radiation

12 APS2012 - Yukawa