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.
arXiv comment13 pages, 13 figures, to appear in EPJC
References in corpus (49)
- An Alternative to Compactification
- f(R) Theories Of Gravity
- Unified cosmic history in modified gravity: from F(R) theory to Lorentz non-invariant models
- f(R) theories
- Extended Theories of Gravity
- f(R,T) gravity
- A Dynamical Solution to the Problem of a Small Cosmological Constant and Late-time Cosmic Acceleration
- k-Inflation
- f(T) teleparallel gravity and cosmology
- Modulus Stabilization with Bulk Fields
- Kinetically Driven Quintessence
- Modeling the fifth dimension with scalars and gravity
- Perturbations in k-inflation
- Universal Aspects of Gravity Localized on Thick Branes
- Gravitational Stability and Renormalization-Group Flow
- Further matters in space-time geometry: gravity
- General Gauss-Bonnet brane cosmology
- Cuscuton: A Causal Field Theory with an Infinite Speed of Sound
- gravity and Cardassian-like expansion as one of its consequences
- Global topological k-defects
- Large-scale cosmological perturbations on the brane
- f(R) gravity theory and CMBR constraints
- Cuscuton Cosmology: Dark Energy meets Modified Gravity
- Cuscuton and low energy limit of Horava-Lifshitz gravity
- f(R)-Brane
- Braneworld solutions for F(R) models with non-constant curvature
- Junction conditions and thin-shells in perfect-fluid gravity
- Configurational entropy in brane models
- K fields, compactons, and thick branes
- Thick brane models in generalized theories of gravity
- Cuscuton Bounce
- Kinematics and Dynamics of Theories of Gravity
- First-order framework and domain-wall/brane-cosmology correspondence
- Thick brane in mimetic gravity
- Fermion localization mechanism with derivative geometrical coupling on branes
- Thick branes with inner structure in mimetic gravity
- Fermions on deformed thick branes
- Thick brane structures in generalized hybrid metric-Palatini gravity
- Theory of Cosmological Perturbations with Cuscuton
- On the many-field f(R) brane
- Cuscuton kinks and branes
- Cosmological Gravitational Wave in a Gravity with Quadratic Order Curvature Couplings
- Information content in brane models with non-constant curvature
- Dressed Power-law Inflation with Cuscuton
- Note on the Gauss-Bonnet braneworld scenario
- Internal structure of cuscuton Bloch brane
- On Higher Derivative Gravity in Two Dimensions
- Hybrid Bloch Brane
- Fundamental energy scale of the thick brane in mimetic gravity