Chameleon Mechanism in Scalar Nonmetricity Cosmology
arXiv:2407.05042 · doi:10.1016/j.aop.2024.169724
Abstract
We investigate the dynamics and the phase-space evolution for the scalar nonmetricity cosmology with a Chameleon mechanism. In particular, we consider a spatially flat Friedmann--Lema\^ıtre--Robertson--Walker geometry and within the framework of scalar nonmetricity theory, we consider a generalization of the Brans-Dicke theory in nonmetricity gravity. Introducing a pressureless gas as the matter source, we also incorporate a coupling function responsible for the interaction. Our findings reveal that the choice of connection in nonmetricity gravity significantly impacts the interaction between the scalar field and the matter source. For one particular connection, we discover the absence of asymptotic solutions with a nontrivial interacting component. More precisely, in this scenario, the matter source does not directly interact with the scalar field; however, there is an interaction with the dynamical degrees of freedom provided by the connection.
28 pages, 4 Figures
References in corpus (10)
- Unified cosmic history in modified gravity: from F(R) theory to Lorentz non-invariant models
- Testing gravity with redshift space distortions
- Quintom cosmologies admitting either tracking or phantom attractors
- Cosmology in gravity: A unified dynamical system analysis at background and perturbation levels
- Dynamics of Quintessence Models of Dark Energy with Exponential Coupling to the Dark Matter
- Observational constraints on two cosmological models of theory
- Phase-space analysis of a novel cosmological model in theory
- Dynamics in interacting scalar-torsion theory
- Phase-space analysis of the viscous fluid cosmological models in the coincident gravity
- Withholding Potentials, Absence of Ghosts and Relationship between Minimal Dilatonic Gravity and f(R) Theories
Cited by in corpus (5)
- The CosmoVerse White Paper: Addressing observational tensions in cosmology with systematics and fundamental physics
- DESI results: Hint towards coupled dark matter and dark energy
- Unexplored regions in teleparallel gravity: Sign-changing dark energy density
- Imprints of screened dark energy on nonlocal quantum correlations
- Can an Extra Degree of Freedom in Scalar-Tensor Non-Metricity Gravity Account for the Evolution of the Universe?