From: utzoo!decvax!cca!gwyn@BRL@sri-unix Newsgroups: net.physics Title: Re: The Hubble Constant Article-I.D.: sri-unix.4349 Posted: Tue Nov 23 16:59:57 1982 Received: Thu Nov 25 06:34:33 1982 From: Doug Gwyn Okay, by way of clarification: The theories of relativity are inherently LOCAL theories, by which is meant that the physical constraints derived from the theories apply to the near vicinity of an observer. To relate distant events to the observer, some extrapolation mechanism is needed, typically path- integration (this immediately leads to considering unified field theory, but that is another topic). The not-faster-than-light constraint applies to a physical object (which can serve as the origin of an inertial system) moving past an observer, in the vicinity of the observer. To measure speeds a significant distance removed from oneself, certain conventions and assumptions must be made. If you try to project your locally-flat space out to cosmological (or in to Schwarzschild) distances using Euclidean intuition, then it is easy to arrive at conclusions in apparent violation of relativistic constraints. The "horizon" is the naively-extrapolated distance at which (according to the idea that the Hubble distance-velocity law holds) one thinks that objects are moving away at the speed of light. However, were you to actually travel a significant percentage of this distance and come to rest with respect to your surroundings, you would find that the horizon has apparently receded such that you still have just as far to go to reach it (which means, of course, that you will never actually get there). This paragraph is stated according to one view of cosmology (the "perfect cosmological principle" DeSitter universe, which is the simplest solution to the Schrodinger field laws). There are actually several peripherally-related matters of interest involved here: 1) The not-faster-than-light injunction; 2) Extrapolation away from the local environment; 3) Integration of differential field laws; 4) Perfect cosmological principle; 5) Einstein-Schrodinger unified field theory. I am willing to discuss these further if you have a particular interest.