External Field Effect in Gravity
arXiv:2103.13972 · doi:10.1142/S0218271821420098
Abstract
In both Newtonian gravity and Einstein gravity there is no force on a test particle located inside a spherical cavity cut out of a static, spherically symmetric mass distribution. Inside the cavity exterior matter is decoupled and there is no external field effect that could act on the test particle. However, for potentials other than the Newtonian potential or for geometries other than Ricci flat ones this is no longer the case, and there then is an external field effect. We explore this possibility in various alternate gravity scenarios, and suggest that such (Machian) external field effects can serve as a diagnostic for gravitational theory.
arXiv comment9 pages, 4 figures. Essay written for the Gravity Research Foundation 2021 Awards for Essays on Gravitation
References in corpus (21)
- Relativistic gravitation theory for the MOND paradigm
- Modified Newtonian Dynamics as an Alternative to Dark Matter
- The Radial Acceleration Relation in Rotationally Supported Galaxies
- Scalar-Tensor-Vector Gravity Theory
- Alternatives to Dark Matter and Dark Energy
- The MOG weak field approximation and observational test of galaxy rotation curves
- Fitting galactic rotation curves with conformal gravity and a global quadratic potential
- Impact of a global quadratic potential on galactic rotation curves
- Are galactic rotation curves really flat?
- The Bullet Cluster 1E0657-558 evidence shows Modified Gravity in the absence of Dark Matter
- The MOG Weak Field approximation II. Observational test of Chandra X-ray Clusters
- Testing the Strong Equivalence Principle: Detection of the External Field Effect in Rotationally Supported Galaxies
- Fundamental parameter-free solutions in Modified Gravity
- Fitting dwarf galaxy rotation curves with conformal gravity
- Modified Gravity (MOG), the speed of gravitational radiation and the event GW170817/GRB170817A
- Modified Gravity (MOG) fits to observed radial acceleration of SPARC galaxies
- NGC 1052-DF2 And Modified Gravity (MOG) Without Dark Matter
- Universal Properties of Galactic Rotation Curves and a First Principles Derivation of the Tully-Fisher Relation
- Modified Gravity (MOG), Cosmology and Black Holes
- Gravitational Theory of Cosmology, Galaxies and Galaxy Clusters
- Limitations of the Standard Gravitational Perfect Fluid Paradigm
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- Imprint of galactic rotation curves and metric fluctuations on the recombination era anisotropy
- Quadratic gravity potentials in de Sitter spacetime from Feynman diagrams