Newtonian approximation in (1 + 1) dimensions
arXiv:2205.12229 · doi:10.1088/1402-4896/ac9e80
Abstract
We study the possible existence of a Newtonian regime of gravity in dimensions, considering metrics in both the Kerr-Schild and conformal forms. In the former case, the metric gives the exact solution of the Poisson equation in flat space, but the weak-field limit of the solutions and the non-relativistic regime of geodesic motion are not trivial. We show that using harmonic coordinates, the metric is conformally flat and a weak-field expansion is straightforward. An analysis of the non-relativistic regime of geodesic motion remains non-trivial and the weak-field potential only satisfies the flat space Poisson equation approximately.
Added references, expanded discussions
References in corpus (12)
- Fractal properties of quantum spacetime
- Dimension and Dimensional Reduction in Quantum Gravity
- When is g_{tt} g_{rr} = -1?
- Detecting Vanishing Dimensions Via Primordial Gravitational Wave Astronomy
- Matter and gravitons in the gravitational collapse
- Dimensional flow in discrete quantum geometries
- Diffusion in quantum geometry
- Evidence for Asymptotic Safety from Dimensional Reduction in Causal Dynamical Triangulations
- Spectral dimensions and dimension spectra of quantum spacetimes
- Effective metric outside bootstrapped Newtonian sources
- Orbits in bootstrapped Newtonian gravity
- Orbits in a stochastic Schwarzschild geometry