Effects of Cuscuton dynamics on braneworld configurations in the scalar-tensor representation of gravity
arXiv:2111.08089 · doi:10.1140/epjc/s10052-022-10196-1
Abstract
In this work we study braneworld configurations in the scalar-tensor representation of the gravity theory in the presence of a Cuscuton term in the source field matter Lagrangian. We start by deriving the scalar-tensor representation of the theory and obtaining its respective equations of motion. We then introduce the standard metric for a flat braneworld model with one extra dimension for the general case of a theory and study two different models for the source field. Given the complexity of the field equations, these solutions are obtained numerically. In these cases, the Cuscuton term effectively amplifies the effect, by increasing the height of the stability potential barrier and, consequently, the depth of the minimum of the graviton zero-mode on the brane. Finally, we study the particular cases of and , for which only the scalar fields or are present, respectively, and we prove that the presence of the scalar field is essential in the development of internal structure on the brane.
13 pages, 13 figures, to appear in EPJC
References in corpus (14)
- Unified cosmic history in modified gravity: from F(R) theory to Lorentz non-invariant models
- f(R,T) gravity
- Cuscuton: A Causal Field Theory with an Infinite Speed of Sound
- Global topological k-defects
- Cuscuton Cosmology: Dark Energy meets Modified Gravity
- Cuscuton and low energy limit of Horava-Lifshitz gravity
- f(R)-Brane
- Junction conditions and thin-shells in perfect-fluid gravity
- K fields, compactons, and thick branes
- Thick brane models in generalized theories of gravity
- First-order framework and domain-wall/brane-cosmology correspondence
- Dressed Power-law Inflation with Cuscuton
- Internal structure of cuscuton Bloch brane
- Hybrid Bloch Brane