Article,

Thick string-like braneworlds in f(T) gravity

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INTERNATIONAL JOURNAL OF MODERN PHYSICS D, (2021)
DOI: 10.1142/S0218271821500474

Abstract

We propose a codimension two warped braneworld model within the teleparallel 1(T) gravity. Asymptotically, the bulk geometry converges to an AdS6 spacetime whose cosmological constant is produced by the torsion parameters. Furthermore, the torsion induces an AdS-dS transition on the exterior region. As the torsion parameters vary, the brane undergoes a phase transition from a thick string-like brane into ring-like structures. The bulk-brane Planck mass ration is modified by the torsion. The analysis of the stress-energy condition reveals a splitting brane process satisfying the weak and strong-energy conditions for some values of the parameters. In addition, we investigate t he behavior of the gravitational perturbations in this scenario. It turns out that the gravitational spectrum has a linear behavior for small masses and is independent of the torsion parameters for large masses. In the bulk, the torsion keeps a gapless nonlocalizable and stable tower of massive modes. Inside the brane core, the torsion produces new barriers and potential wells leading to small amplitude massive modes and a massless mode localized around the ring structures. We propose a codimension two warped braneworld model within the teleparallel f(T) gravity. Asymptotically, the bulk geometry converges to an AdS(6) spacetime whose cosmological constant is produced by the torsion parameters. Furthermore, the torsion induces an AdS-dS transition on the exterior region. As the torsion parameters vary, the brane undergoes a phase transition from a thick string-like brane into ring-like structures. The bulk-brane Planck mass ration is modified by the torsion. The analysis of the stress-energy condition reveals a splitting brane process satisfying the weak and strong-energy conditions for some values of the parameters. In addition, we investigate t he behavior of the gravitational perturbations in this scenario. It turns out that the gravitational spectrum has a linear behavior for small masses and is independent of the torsion parameters for large masses. In the bulk, the torsion keeps a gapless nonlocalizable and stable tower of massive modes. Inside the brane core, the torsion produces new barriers and potential wells leading to small amplitude massive modes and a massless mode localized around the ring structures.

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