Relay-Version: version B 2.10 5/3/83; site utzoo.UUCP Path: utzoo!watmath!clyde!burl!ulysses!gamma!epsilon!zeta!sabre!petrus!bellcore!decvax!decwrl!pyramid!pesnta!phri!cmcl2!lanl!jlg From: jlg@lanl.ARPA (Jim Giles) Newsgroups: net.physics Subject: Re: Coordinate frames in GR Message-ID: <1035@lanl.ARPA> Date: Thu, 27-Mar-86 19:43:47 EST Article-I.D.: lanl.1035 Posted: Thu Mar 27 19:43:47 1986 Date-Received: Sat, 29-Mar-86 06:13:34 EST References: <438@batcomputer.TN.CORNELL.EDU> <1005@lanl.ARPA> Reply-To: jlg@a.UUCP (Jim Giles) Organization: Los Alamos National Laboratory Lines: 116 People who have been following this discussion are aware that I have, so far, tried to keep the discussion general enough for the layman to follow (at least, roughly). I have avoided using terms like 'Kerr- Newman geometry' and 'Minkowski spaces' in order not to lose the average reader in a cloud of opaque terminology. I continue this effort, in spite of attempts by others on the net to obscure what should be a simple point. To reintroduce the subject: Matt Weiner of Berkeley has been defending the statement by Bertrand Russell that rotation of the Earth vs. rotation of the universe around the Earth is 'merely' a matter of convenience. I think Russell was just being a little over-zealous in his support of relativism here, Weiner is being more than over-zealous - he is being obstinate. Part I. below gives a summary of my position with no complex terminology and no coordinate systems. I. Consider an isolated region of space distant from any large masses. The geometry of space-time is flat in this region for most practical purposes. Vibrating test particles (ie. pendula) appear to co-rotate with respect to the distant stars. Spinning test particles (ie. gyroscopes) appear to have a fixed axis with respect to the distant stars. Consider, now, another isolated region which is a few Giga-parsecs from the first. Again, the same observations of test particles give the same observations. In addition, any observer who can see BOTH sets of experiments will notice that the test particles co-rotate with each other as well as the stars distant from each. That is, pendula and gyroscopes precess identically - even if seperated by large distances. But, this can't have any significance. Matt Weiner from Berkeley says it doesn't :-). Last week, Matt Weiner posted an article which quoted a passage from 'Gravitation' by Mizner, Thorne, and Wheeler. To make my point clear, I will reproduce the passage in question here: 'In spacetime the intervals ("proper distance," "proper time") between event and event satisfy the corresponding theorems of Lorentz-Minkowski geometry (Box 1.3). These theorems lend themselves to empirical test in the appropriate, very special coordinate systems: [...] (local Lorentz coordinates; local inertial frame) in the local Lorentz geometry of physics. However, these theorems rise above all coordinate systems in their content. They refer to intervals and distances.' (The Lorentz geometry is being introduced in analogy to Euclidean geometry, hence the term 'corresponding'.) Mr. Weiner, in his commentary on this passage, made the claim that the theorems in question (those of the Lorentz-Minkowski geometry) applied equally to ALL coordinate systems. This is not true (particularly for the equations in box 1.3, which apply correctly only to Lorentz frames - that is, local inertial reference frames when orthonormal coordinates are used). To make this clear, consider sections II. and III. below. II. Consider the same sort of isolated region. Along come two experimenters. They decide (for their own reasons) that they need a coordinate system fo physical measurements of their experiments. Since the local region of space-time is flat (ie. Lorentzian) they both decide to use a Lorentz frame as their coordinate system. The first experimenter has been reading this discussion on galaxy-net, and decides that, since rotation is merely a matter of convenience, he will fix his 'frame' to his rotating spacecraft (it's rotating to prevent his equipment from floating about the lab in an inconvenient way :-). Now, Matt Weiner has assured him that the formulae in Box 1.3 of 'Gravitation' apply to ANY coordinate system - including rotating ones. These are the equations of Special Relativity. This first experimenter then proceeds to make his measurements and finds, to his surprise, that they are inconsistent! His conclusion is that either Special Relativity is wrong, or Matt Weiner is. "But, Matt Weiner can't be wrong," he thinks, "he's from Berkeley!" He now proceeds down a trail of increasingly confusing, incorrect, and inconsistent reasoning from which there is no escape. III. Experimenter number two also goes through the same reasoning. But, when he finds his results are inconsistent, he thinks: "Maybe this Weiner guy has a screw loose (from spending too much time getting dizzy in rotating coordinate systems no doubt :-). Maybe there IS a significant difference between rotating and non- rotating coordinate systems." The second experimenter then repeats his observations in a Lorentzian frame which co-rotates with the distant stars (and his local pendula, etc.). Now he finds that his results are consistent with predictions of Special Relativity. Now he thinks: "Gee, rotation was not a matter of 'mere' convenience after all. There is a significant effect here." I owe an apology to those readers of the net who have had to wade through this discussion for an extra week. I noticed the errors in Mr. Weiner's submission when I first read it. But, since he included with it a lot of ad-hominem abuse directed at me, I thought it would be fun to watch him try to extract his foot from his mouth. In the interest of this, I gave a number of blatant clues that his submission was incorrect: but he seems to be unaware that the tough bony thing he's chewing is his foot. For anyone who has been struggling though this debate (especially those who obtained a copy of 'Gravitation'), I would like to assure you that the equations of Special Relativity are obeyed only within local inertial reference frames. And, especially, the equations in Box 1.3 of 'Gravitation' are obeyed only within Lorentz frames (ie. local frames with orthonormal coordinates). To apply these equations to any other coordinate systems would require mathematical tools which are quite beyond the scope of Special Relativity (though, well within the grasp of General Relativity). This is not to say that these mathematical tools are too complex to be handled in Special Relativity: Newton would probably have understood how to transform from a rotating coordinate system to a non-rotating one. It's just that these techniques are not part of the relevant subject matter of Special Relativity. J. Giles Los Alamos