Relay-Version: version B 2.10 5/3/83; site utzoo.UUCP Posting-Version: version B 2.10.1 6/24/83; site charm.UUCP Path: utzoo!watmath!clyde!burl!ulysses!mhuxr!mhuxn!charm!grl From: grl@charm.UUCP (George Lake) Newsgroups: net.physics Subject: Re: the multi-body problem Message-ID: <762@charm.UUCP> Date: Mon, 30-Sep-85 13:22:24 EDT Article-I.D.: charm.762 Posted: Mon Sep 30 13:22:24 1985 Date-Received: Thu, 3-Oct-85 04:02:23 EDT References: <1330@teddy.UUCP> Organization: Physics Research @ AT&T Bell Labs Murray Hill NJ Lines: 17 The two-body problem is exceedlingly simple. You can solve the equations of both particles by considering their motion in the center of mass frame. Conservation of momentume insures that the center of mass moves at a constant velocity. Then the two particles perform symmetric motions about this point. The entire motion lies in a plane in this frame. In some deep sense this occurs because the "1-body" problem in a central force is so very simple. Most potentials have 3 distinct invariants of motion. The central force has 4, the Kepler problem has 5. This super-integrability makes the next higher problem tractable. At three it goes away. One way to see it is in terms of resonance. Two particles orbit one another with a single frequency. Three particles have multiple frequencies. When the frequencies are equal, resonance makes the motion wild and difficult to calculate. There are infinitely many resonances that all have be calculated. Each resonance is a singularity and perturbation calculations won't go through them. Brought to you by Super Global Mega Corp .com