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2007

Bubbles in the Self-Accelerating Universe

Izumi, Keisuke, Koyama, Kazuya, Pujolas, Oriol et al.

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We revisit the issue of the stability in the Dvali-Gabadadze-Porrati model, by considering the nucleation of bubbles of the conventional branch within the self-accelerating branch.

We construct an instanton describing this process in the thin wall approximation.
On one side of the bubble wall, the bulk consists of the exterior of the brane while on the other side it is the interior.
The solution requires the presence of a 2-brane (the bubble wall) which induces the transition.

Bubbles in the Self-Accelerating Universe · Around

Built on

G. Gabadadze, arXiv:hep-th/0612213; arXiv:0705.1929 [hep-th]
Original
1929
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S. R. Coleman and F. De Luccia, Phys. Rev. D 21
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N. Kaloper, Phys. Rev. D 71
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E. Witten, Nucl. Phys. B 195
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The way how we interpret a gravitational instanton here is explained in e.g. T. Tanaka and M. Sasaki Prog. Theor. Phys. 88
1992
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G. R. Dvali, G. Gabadadze and M. Porrati, Phys. Lett. B 484
2000
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C. Deffayet, Phys. Lett. B 502
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K. Izumi, K. Koyama and T. Tanaka, arXiv:hep-th/0610282

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