Gravitational interactions in a general multibrane model

Jolyon K. Bloomfield and Éanna É. Flanagan
Phys. Rev. D 84, 104016 – Published 7 November 2011

Abstract

The gravitational interactions of the four-dimensional effective theory describing a general N-brane model in five dimensions without radion stabilization are analyzed. Both uncompactified and orbifolded models are considered. The parameter space is constrained by requiring that there be no ghost modes in the theory, and that the Eddington parametrized post-Newtonian parameter γ be consistent with observations. We show that we must reside on the brane on which the warp factor is maximized. The resultant theory contains N1 radion modes in a nonlinear sigma model, with the target space being a subset of hyperbolic space. Imposing observational constraints on the relative strengths of gravitational interactions of dark and visible matter shows that at least 99.8% of the dark matter must live on our brane in this model.

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  • Received 26 January 2011

DOI:https://doi.org/10.1103/PhysRevD.84.104016

© 2011 American Physical Society

Authors & Affiliations

Jolyon K. Bloomfield*

  • Physics Department, Cornell University, Ithaca, New York 14853, USA

Éanna É. Flanagan

  • Center for Radiophysics and Space Research, Cornell University, Ithaca, New York 14853, USA and Newman Laboratory for Elementary Particle Physics, Cornell University, Ithaca, New York 14853, USA

  • *jkb84@cornell.edu
  • flanagan@astro.cornell.edu

See Also

Four-dimensional description of five-dimensional N-brane models

Jolyon K. Bloomfield and Éanna É. Flanagan
Phys. Rev. D 82, 124013 (2010)

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Vol. 84, Iss. 10 — 15 November 2011

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