
arXiv: 1012.5298
We consider a 5D warped scenario with a KK-parity symmetry, where the non-trivial warping arises from the dynamics that stabilizes the size of the extra dimension. Generically, the lightest Kaluza-Klein (KK) particle is the first excitation of the radion field, while the next-to-lightest Kaluza-Klein particle is either the first excitation of the (RH) top quark or the first KK-parity odd Higgs. All these masses are expected to be of order the electroweak scale. We present simple analytical expressions for the masses and wavefunctions of the lowest lying KK modes, and derive the Feynman rules necessary for phenomenological applications. The framework allows to interpolate between a strongly warped scenario a la Randall-Sundrum (RS), and a weakly warped scenario that shares properties of both RS and Universal Extra Dimensions models.
41 pages, 13 figures. Minor comments added. Published version
High Energy Physics - Theory, field theories in higher dimensions, FOS: Physical sciences, Quantum field theory on curved space or space-time backgrounds, Two-dimensional field theories, conformal field theories, etc. in quantum mechanics, Finite-dimensional groups and algebras motivated by physics and their representations, High Energy Physics - Phenomenology, AdS-CFT correspondence, High Energy Physics - Phenomenology (hep-ph), High Energy Physics - Theory (hep-th), Unified quantum theories, Geometrodynamics and the holographic principle, beyond standard model, cosmology of theories beyond the SM, Feynman diagrams, Relativistic cosmology
High Energy Physics - Theory, field theories in higher dimensions, FOS: Physical sciences, Quantum field theory on curved space or space-time backgrounds, Two-dimensional field theories, conformal field theories, etc. in quantum mechanics, Finite-dimensional groups and algebras motivated by physics and their representations, High Energy Physics - Phenomenology, AdS-CFT correspondence, High Energy Physics - Phenomenology (hep-ph), High Energy Physics - Theory (hep-th), Unified quantum theories, Geometrodynamics and the holographic principle, beyond standard model, cosmology of theories beyond the SM, Feynman diagrams, Relativistic cosmology
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