Spherically symmetric solution of gravity at low energy
arXiv:1510.08552 · doi:10.1103/PhysRevD.92.044012
Abstract
The weak-field and slow-motion limit of gravity is developed up to order in a spherically symmetric background. Considering the Taylor expansion of a general function around vanishing values of and , we present general vacuum solutions up to order for the gravitational field generated by a ball-like source. The spatial behaviors at order are the same for gravity and gravity, and their corresponding real valued static behaviors are presented and compared with the one in general relativity. The static Yukawa-like behavior is proved to be compatible with the previous result of the most general fourth-order theory. At order, the static corrections to the Yukawa-like behavior for gravity, gravity, and the Starobinsky gravity are presented and compared with the one in general relativity.
14 latex files, 11 figures
References in corpus (14)
- Unified cosmic history in modified gravity: from F(R) theory to Lorentz non-invariant models
- Low surface brightness galaxies rotation curves in the low energy limit of gravity : no need for dark matter?
- Limit to General Relativity in f(R) theories of gravity
- The Newtonian Limit of F(R) gravity
- Dark energy and dark matter as curvature effects
- Spherical symmetry in -gravity
- Ghosts, Instabilities, and Superluminal Propagation in Modified Gravity Models
- Dark matter and dark energy as a effects of Modified Gravity
- Ghost Constraints on Modified Gravity
- A general solution in the Newtonian limit of f(R)- gravity
- Starobinsky-type Inflation in Dynamical Supergravity Breaking Scenarios
- The Newtonian limit of metric gravity theories with quadratic Lagrangians
- The most general fourth order theory of Gravity at low energy
- Cosmological entropy and generalized second law of thermodynamics in theory of gravity
Cited by in corpus (8)
- Noether Symmetry Approach in Gravity
- Observational constrained gravity cosmological model and the dynamical system analysis
- Cosmological model with time varying deceleration parameter in gravity
- Multipole analysis for linearized gravity with irreducible Cartesian tensors
- Multipole analysis for linearized gravity with irreducible Cartesian tensors
- The gravitational field outside a spatially compact stationary source in a generic fourth-order theory of gravity
- Scale-Invariant Bounce Cosmology in Weyl f(Q) Gravity with Quintom Signature
- Late-Time Cosmic Acceleration in Ricci-Gauss-Bonnet Gravity via Gradient Descent Optimization