Radion dynamics and electroweak physics

Csaba Csáki, Michael L. Graesser, and Graham D. Kribs
Phys. Rev. D 63, 065002 – Published 1 February 2001
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Abstract

The dynamics of a stabilized radion in the Randall-Sundrum model with two branes is investigated, and the effects of the radion on electroweak precision observables are evaluated. The radius is assumed to be stabilized using a bulk scalar field as suggested by Goldberger and Wise. First the mass and the wave function of the radion is determined including the back reaction of the bulk stabilization field on the metric, giving a typical radion mass of the order of the weak scale. This is demonstrated by a perturbative computation of the radion wave function. A consequence of the background configuration for the scalar field is that after including the back reaction the Kaluza-Klein states of the bulk scalars couple directly to the standard model fields on the TeV brane. Some cosmological implications are discussed, and in particular it is found that the shift in the radion at late times is in agreement with the four-dimensional effective theory result. The effect of the radion on the oblique parameters is evaluated using an effective theory approach. In the absence of a curvature-scalar Higgs mixing operator, these corrections are small and give a negative contribution to S. In the presence of such a mixing operator, however, the corrections can be sizable due to the modified Higgs and radion couplings.

  • Received 29 August 2000

DOI:https://doi.org/10.1103/PhysRevD.63.065002

©2001 American Physical Society

Authors & Affiliations

Csaba Csáki*

  • Theory Division T-8, Los Alamos National Laboratory, Los Alamos, New Mexico 87545

Michael L. Graesser

  • Department of Physics, University of California, Santa Cruz, California 95064

Graham D. Kribs

  • Department of Physics, Carnegie Mellon University, Pittsburgh, Pennsylvania 15213

  • *Email address: csaki@lanl.gov
  • Email address: graesser@scipp.ucsc.edu
  • Present address: Department of Physics, University of Wisconsin, Madison, WI 53706. Email address: kribs@pheno.physics.wisc.edu

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Issue

Vol. 63, Iss. 6 — 15 March 2001

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