Dynamics of self-gravitating systems in non-linearly magnetized chameleonic Brans-Dicke gravity
arXiv:2301.07105 · doi:10.1007/s10714-023-03071-1
Abstract
We study the effects of magnetic fields of non-linear electrodynamics in chameleonic Brans-Dicke theory under the existence of anisotropic spherical fluid. In particular, we explore dissipative and non-dissipative self-gravitating systems in the quasi-homologous regime with the minimal complexity constraint. As a result, under the aforementioned circumstances, several analytic solutions are found. Furthermore, by analyzing the dynamics of a dissipative fluid, it is demonstrated that a void covering the center can satisfy the Darmois criteria. The temperature of the self gravitating systems is also investigated.
26 pages, version accepted for publication in General Relativity and Gravitation
References in corpus (12)
- Integrated Sachs-Wolfe effect from the cross correlation of WMAP3 year and the NRAO VLA sky survey data: New results and constraints on dark energy
- CP Violation in Leptonic Rare Decays as a Probe of New Physics
- Extragalactic Radio Sources and the WMAP Cold Spot
- Cosmological Effects of Nonlinear Electrodynamics
- Holographic dark energy in Brans-Dicke cosmology with chameleon scalar field
- Quasi-homologous evolution of self-gravitating systems with vanishing complexity factor
- Interacting HDE and NADE in Brans-Dicke Chameleon Cosmology
- The Holographic Model of Dark Energy and Thermodynamics of Non-Flat Accelerated Expanding Universe
- Decaying Gravity
- Role of gravitational decoupling on isotropization and complexity of self-gravitating system under complete geometric deformation approach
- Screening Mechanism and Late-time Cosmology: Role of a Chameleon-Brans-Dicke Scalar Field
- Energy conditions in a modified Brans-Dicke theory