Bubble Nucleation and Eternal Inflation - cosmo 06

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Bubble Nucleation and Eternal Inflation - cosmo 06

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C

r

III’’

III I

C

III’’

IV

II’’

IV’’

r C

III''

II’’

r C

Two

III

Tunnels

I

III'

II

IV''

IV

IV'

r C

BH

r BH

rBH

BH

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FIG. 10: Conformal diagrams for the thermalon spacetime

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and F. De Luccia, Phys. Rev. D21, 3305 (1980).

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II

II’

[6]

IV’’

D. J. Gross, M. J. Perry, andIV

L. G. Yaffe, Phys. Rev. D25,

IV’

330 (19

[7] P. H. Ginsparg and M. J. Perry, Nucl. Phys. B222, 245 (1983).

I

III’

[8] R. III Bousso and A. Chamblin, Phys. Rev. D59, 084004 (1999), gr-qc

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FIG. IV 11: Tunneling through IV’ the worm hole.

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FIG. 11: Tunneling through the worm hole.

R Tunneling Geometry: goes through dS horizon.

[14] R. II Basu, A. II’ H. Guth, and II’’ A. Vilenkin, Phys. Rev. D44, 340 (1991)

[15] I

III A. Aurilia, M. Palmer, III’ and E. Spallucci, Phys. Rev. D40, 2511 (198

III

r

BH

r C

L Tunneling Geometry: goes through wormhole.

II

IV

r

r C

BH

[18] T. FIG. R. 12: Choudhury Second option for tunneling. and T. Padmanabhan (2004), gr-qc/0404091.

[20] B. Freivogel 9 et al. (2005), hep-th/0510046.

I

II’

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IV

IV’

IV’’

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IV’

[19] F.-L. Lin and C. Soo, Class. Quant. Grav. 16, 551 (1999), gr-qc/97

r BH

r C

III’

FIG. 12: Second option for tunneling.

II’’

IV’’

II’

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