Hamilton-Jacobi method for curved domain walls and cosmologies - INSPIRE

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Hamilton-Jacobi method for curved domain walls and cosmologies

Sep, 2006

18 pages

Published in:

Phys.Rev.D 74 (2006) 125008

e-Print:

hep-th/0609056 [hep-th]

DOI:

10.1103/PhysRevD.74.125008

Report number:

ITFA-2006-32

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Abstract: (arXiv)

We use Hamiltonian methods to study curved domain walls and cosmologies. This leads naturally to first order equations for all domain walls and cosmologies foliated by slices of maximal symmetry. For Minkowski and AdS-sliced domain walls (flat and closed FLRW cosmologies) we recover a recent result concerning their (pseudo)supersymmetry. We show how domain-wall stability is consistent with the instability of adS vacua that violate the Breitenlohner-Freedman bound. We also explore the relationship to Hamilton-Jacobi theory and compute the wave-function of a 3-dimensional closed universe evolving towards de Sitter spacetime.

11.27.+d
98.80.Jk
04.65.+e
domain wall: stability
Hamilton-Jacobi equation
Hamiltonian formalism
space-time: anti-de Sitter
supersymmetry
wave function: semiclassical

References(22)

Figures(0)

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