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Bent Domain Walls as Braneworlds

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arxiv hep-th/9905210 v3 pith:FBXV6DQQ submitted 1999-05-27 hep-th astro-phgr-qchep-ph

classification hep-thastro-phgr-qchep-ph
keywords wallssolutionswallconstantcurvaturedomainmuchtension
verification ladder T0 review T1 audit T2 compute T3 formal

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We consider domain walls embedded in curved backgrounds as an approximation for braneworld scenarios. We give a large class of new exact solutions, exhausting the possibilities for describing one and two walls for the cases where the curvature of both the bulk and the wall is locally constant. In the case of two walls, we find solutions where each wall has positive tension. An interesting property of these solutions is that the curvature of the walls can be much smaller than the tension, leading to a significant cancellation of the effective cosmological constant, which however is still much larger than the observational limits. We further discuss some aspects of inflation in models based on wall solutions.

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Cited by 4 Pith papers

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    Radion dynamics in warped 5D models enhance the axion decay constant during inflation, satisfying CMB isocurvature bounds at higher Hubble scales while restoring the QCD window afterward.

  3. Inflation with a Growing Fifth Dimension

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    Inflation from a UV-brane inflaton in a warped 5D bulk with an IR brane predicts a blue-tilted low-k scalar spectrum and oscillating tensor features because the early adiabatic modes come from the radion.

  4. Quasinormal Ringing of de Sitter Braneworlds

    gr-qc 2024-12 conditional novelty 6.0 of 10

    Thin and thick de Sitter braneworlds have discrete, purely imaginary quasinormal frequencies for gravitational perturbations, with decay rates set by the Hubble constant and, for thick branes, by the brane width parameter.

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