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Static brane solutions stabilized by nonlinear bulk scalar dynamics

Sunnyeo Lee1, Tae Hoon Lee1, Joohan Lee2 and Phillial Oh3

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We study a nonlinear sigma-model-like theory of a bulk scalar field coupled to the five-dimensional Einstein gravity with a negative cosmological constant. We determine the structure of the non-factorizable spacetime which our Minkowskian brane bounds, when the pressure in the extra dimension is proportional to the energy density of the scalar field as \tilde{p}_5=\omega _5 \tilde{\rho } with a constant ω5. With these static solutions clarified by the parameter ω5, we fix the size of the extra dimension in terms of the bulk and brane potentials of the scalar field, imposing the stability condition in the cases of the 2-branes. The hierarchy problem is discussed in their Randall–Sundrum-like limit, and one of the static solutions obtained in the case of a strong bulk potential ω5 < 0 is interpreted as a thick 1-brane model.


PACS

04.50.-h Higher-dimensional gravity and other theories of gravity

98.80.Cq Particle-theory and field-theory models of the early Universe (including cosmic pancakes, cosmic strings, chaotic phenomena, inflationary universe, etc.)

11.10.Lm Nonlinear or nonlocal theories and models

04.20.Jb Exact solutions

95.30.Sf Relativity and gravitation

MSC

85A40 Cosmology (For relativistic cosmology, see 83F05)

83F05 Cosmology

83C05 Einstein's equations (general structure, canonical formalism, Cauchy problems)

Subjects

Gravitation and cosmology

Particle physics and field theory

Astrophysics and astroparticles

Dates

Issue 24 (21 December 2009)

Received 28 August 2009, in final form 19 October 2009

Published 16 November 2009



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