English

Local and global gravity

General Relativity and Quantum Cosmology 2010-11-30 v1 Astrophysics

Abstract

Our long experience with Newtonian potentials has inured us to the view that gravity only produces local effects. In this paper we challenge this quite deeply ingrained notion and explicitly identify some intrinsically global gravitational effects. In particular we show that the global cosmological Hubble flow can actually modify the motions of stars and gas within individual galaxies, and even do so in a way which can apparently eliminate the need for galactic dark matter. Also we show that a classical light wave acquires an observable, global, path dependent phase in traversing a gravitational field. Both of these effects serve to underscore the intrinsic difference between non-relativistic and relativistic gravity.

Keywords

Cite

@article{arxiv.gr-qc/9611038,
  title  = {Local and global gravity},
  author = {Philip D. Mannheim},
  journal= {arXiv preprint arXiv:gr-qc/9611038},
  year   = {2010}
}

Comments

LaTeX, 20 pages plus three figures in two postscript files. To appear in a special issue of Foundations of Physics honoring Professor Lawrence Horwitz on the occasion of his 65th birthday; A. van der Merwe and S. Raby, Editors, Plenum Publishing Company, N.Y., 1997