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| Tags: acclerations, curvature, flat, space, time |
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#1
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One of the problems I have never resolved is the difference between
curvature and accelerations in flat space-time. I suspect that I'm not wording that quite right, but let me explain what I mean. Given a lab frame resting on a non-rotating earth. Is this frame equivalent, (equally relevent to make predictions and conduct experiments), as a frame accelerating at 9.80 m/s^2 located in space far from any gravity source. The answer I keep getting is _no_. Let me explain why . Let both frames have identical systems of inertially moving objects. In the frame located on the non-rotating earth, the objects all accelerate by varying quantity wrt to the lab and all accelerate with respect to each other. In the frame located away from any source of gravity, the objects all accelerate by identical quantity wrt the lab and all move inertially wrt to each other. So the labs are not identical nor do the paths of their geodesics match in both frames, meaning that, for precise predictions, one must know the actual physical situation of his lab, ie, whether he resting on the launch pad or exiting the solar system with rockets propelling him. I have taken this to mean that there is a fundamental difference between the motions of the objects and the frames. In fact, it would seem, physically, that they are precisely the opposite of each other, a mirror image so to speak. Welcome any and all comments. Phil |
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#2
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Phil wrote:
One of the problems I have never resolved is the difference between curvature and accelerations in flat space-time. [...] There has been no experimental proof to indicate a centripetal time dilation. So much for Einstein's Equivalence Principle! |
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#3
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Koobee Wublee wrote: Phil wrote: One of the problems I have never resolved is the difference between curvature and accelerations in flat space-time. [...] There has been no experimental proof to indicate a centripetal time dilation. So much for Einstein's Equivalence Principle! Psst...Nobody expects centripetal time dilation. ****, this is even worked out in MTW's _Gravitation_. Specifically, it is shown there is *no* redshift and thus no time dilation. Why is it you can't even get the simple stuff right? The equivalence principle has no bearing on this. |
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#4
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Phil wrote: One of the problems I have never resolved is the difference between curvature and accelerations in flat space-time. I suspect that I'm not wording that quite right, but let me explain what I mean. Given a lab frame resting on a non-rotating earth. Is this frame equivalent, (equally relevent to make predictions and conduct experiments), as a frame accelerating at 9.80 m/s^2 located in space far from any gravity source. The answer I keep getting is _no_. Let me explain why . I don't see why it would be different, barring obvious objections like locality and tidal effects. This is the equivalence principle in action, imho. Let both frames have identical systems of inertially moving objects. In the frame located on the non-rotating earth, the objects all accelerate by varying quantity wrt to the lab and all accelerate with respect to each other. In the frame located away from any source of gravity, the objects all accelerate by identical quantity wrt the lab and all move inertially wrt to each other. So the labs are not identical nor do the paths of their geodesics match in both frames, meaning that, for precise predictions, one must know the actual physical situation of his lab, ie, whether he resting on the launch pad or exiting the solar system with rockets propelling him. I think you are right in this sense. If you break the locality condition, you won't get an inertial frame of reference and everything goes to hell. I have taken this to mean that there is a fundamental difference between the motions of the objects and the frames. In fact, it would seem, physically, that they are precisely the opposite of each other, a mirror image so to speak. Welcome any and all comments. I don't see how you can conclude there is a difference between the object's motion and the object's frame of reference. Phil |
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#5
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"Phil" wrote in message ink.net... One of the problems I have never resolved is the difference between curvature and accelerations in flat space-time. I suspect that I'm not wording that quite right, but let me explain what I mean. Try reading this. http://xxx.lanl.gov/abs/physics/0204044 It is a paper I wrote a few years back. The intent of the paper is to directly answer your question. Given a lab frame resting on a non-rotating earth. Is this frame equivalent, (equally relevent to make predictions and conduct experiments), as a frame accelerating at 9.80 m/s^2 located in space far from any gravity source. The answer I keep getting is _no_. Let me explain why . Let both frames have identical systems of inertially moving objects. In the frame located on the non-rotating earth, the objects all accelerate by varying quantity wrt to the lab and all accelerate with respect to each other. In the frame located away from any source of gravity, the objects all accelerate by identical quantity wrt the lab and all move inertially wrt to each other. So the labs are not identical nor do the paths of their geodesics match in both frames, meaning that, for precise predictions, one must know the actual physical situation of his lab, ie, whether he resting on the launch pad or exiting the solar system with rockets propelling him. This is because you're thinking of a field with tidal accelerations. The Equivalence Principle, as stated by Einstein, is this: A uniformly accelerated frame of reference is identical to a *uniform gravitational field*. For a field which has tidal forces it is to be applied *locally* which means your measurement equipment does not have the precision to tell the difference. E.g. drop a ball in your room and measure its acceleration. The measurement is done with finite precision. Measure its instantanious acceleration at the location of release. Now do the same thing at a point closer to the floor. You'll see that with certain measurement devices that there is no difference in the acceleration. Bringing in more precise measurement devices only means that you're doing the experiments more locally, i.e. within a smaller region of spacetime. Best wishes Pete |
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#6
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"Eric Gisse" wrote in message oups.com... Phil wrote: Let both frames have identical systems of inertially moving objects. In the frame located on the non-rotating earth, the objects all accelerate by varying quantity wrt to the lab and all accelerate with respect to each other. In the frame located away from any source of gravity, the objects all accelerate by identical quantity wrt the lab and all move inertially wrt to each other. So the labs are not identical nor do the paths of their geodesics match in both frames, meaning that, for precise predictions, one must know the actual physical situation of his lab, ie, whether he resting on the launch pad or exiting the solar system with rockets propelling him. I think you are right in this sense. If you break the locality condition, you won't get an inertial frame of reference and everything goes to hell. Well the labs are not inertial by definition. But then, I have the sense that "locality" isn't meaningful anyway. By this I mean that I don't think the difference between the two accelerated frames disappear in an interval of infinitesimal domain. Here is why. The geodesics are the integrations of the contributions of each infinitesmal interval. If the geodesics differ, there must be some difference in the infinitesimal contributions. In other words, to be different in larger domains is to be different infinitesimally, or vice versa. Another way of saying this is that if they were identical infinetesimally, they would integrate identically, resulting in identical motions wrt to the accelerating lab frames. But then, we know that the motions are distinguishable experimentally. I have taken this to mean that there is a fundamental difference between the motions of the objects and the frames. In fact, it would seem, physically, that they are precisely the opposite of each other, a mirror image so to speak. Welcome any and all comments. I don't see how you can conclude there is a difference between the object's motion and the object's frame of reference. In re-reading what I posted, I can understand the confusion you are having with what I said. I meant something entirely different than what you inferred. I'll try to do a better job. The the "inertial" objects are "all moving inertially wrt each other" and "accelerating identically" wrt to the accelerating lab far from a gravity source. While in the accelerating lab resting on the surface of the planet, the "inertial objects are all "accelerating with respect to each other" and "accelerating differently" wrt the lab frame. Physically, they seem to be opposites, that is, in terms of the qualities of their necessary motions. Is this clearer? Phil |
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#7
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"Pete" wrote in message ... "Phil" wrote in message ink.net... One of the problems I have never resolved is the difference between curvature and accelerations in flat space-time. I suspect that I'm not wording that quite right, but let me explain what I mean. Try reading this. http://xxx.lanl.gov/abs/physics/0204044 It is a paper I wrote a few years back. The intent of the paper is to directly answer your question. Given a lab frame resting on a non-rotating earth. Is this frame equivalent, (equally relevent to make predictions and conduct experiments), as a frame accelerating at 9.80 m/s^2 located in space far from any gravity source. The answer I keep getting is _no_. Let me explain why . Let both frames have identical systems of inertially moving objects. In the frame located on the non-rotating earth, the objects all accelerate by varying quantity wrt to the lab and all accelerate with respect to each other. In the frame located away from any source of gravity, the objects all accelerate by identical quantity wrt the lab and all move inertially wrt to each other. So the labs are not identical nor do the paths of their geodesics match in both frames, meaning that, for precise predictions, one must know the actual physical situation of his lab, ie, whether he resting on the launch pad or exiting the solar system with rockets propelling him. This is because you're thinking of a field with tidal accelerations. The Equivalence Principle, as stated by Einstein, is this: A uniformly accelerated frame of reference is identical to a *uniform gravitational field*. For a field which has tidal forces it is to be applied *locally* which means your measurement equipment does not have the precision to tell the difference. E.g. drop a ball in your room and measure its acceleration. The measurement is done with finite precision. Measure its instantanious acceleration at the location of release. Now do the same thing at a point closer to the floor. You'll see that with certain measurement devices that there is no difference in the acceleration. Bringing in more precise measurement devices only means that you're doing the experiments more locally, i.e. within a smaller region of spacetime. Best wishes Pete Thanks Pete for the link, I have downloaded it, and will be reading it forthwith. I fully agree that the difference (the curvature) is a consequence of the non-uniformity of the gravity field (tidal accerations). Since the tidal accelerations are not insignificant, how are they incorporated for predicting paths of motion? It would not be sufficient to integrate the effects under a strict equivalence principle. Phil |
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#8
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"Pete" wrote in message ... Try reading this. http://xxx.lanl.gov/abs/physics/0204044 It is a paper I wrote a few years back. The intent of the paper is to directly answer your question. And I think it does. I found it a very satisfying read. I would like to add that while MGR does seem to add the concept of curvature to Einstein's definition of gravity, it is reasonable from this perspective. Gravity, (as a field of matter/energy), is never devoid of curvature, in as much that the concept of "uniform field" is an idealization for which we have no evidence to exist anywhere in nature, though it may certainly be conceived to be approachable, in that the effects of said curvature, become immeasurable. Reading the historical references of Einstein's papers, I can not help but to be reminded of the wonderful, tounge in cheek way, Einstein approached his physics. Refreshing indeed. Phil |
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#9
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Phil wrote: "Eric Gisse" wrote in message oups.com... Phil wrote: Let both frames have identical systems of inertially moving objects. In the frame located on the non-rotating earth, the objects all accelerate by varying quantity wrt to the lab and all accelerate with respect to each other. In the frame located away from any source of gravity, the objects all accelerate by identical quantity wrt the lab and all move inertially wrt to each other. So the labs are not identical nor do the paths of their geodesics match in both frames, meaning that, for precise predictions, one must know the actual physical situation of his lab, ie, whether he resting on the launch pad or exiting the solar system with rockets propelling him. I think you are right in this sense. If you break the locality condition, you won't get an inertial frame of reference and everything goes to hell. Well the labs are not inertial by definition. But then, I have the sense that "locality" isn't meaningful anyway. By this I mean that I don't think the difference between the two accelerated frames disappear in an interval of infinitesimal domain. Here is why. The geodesics are the integrations of the contributions of each infinitesmal interval. If the geodesics differ, there must be some difference in the infinitesimal contributions. In other words, to be different in larger domains is to be different infinitesimally, or vice versa. Geodesics aren't defined in terms of integrations, rather they are defined in terms of how the metric changes. Path length is defined in such a manner though. I'm not sure how to respond to this in general. Yes the frames are different at large scale. The basic point is that at *small* scale you cannot tell the difference if you look at an area so small that it you can construct an inertial coordinate system for the lab frame and so small that you cannot observe tidal effects due to gravity. If those two conditions are satisfied, you can't tell the difference between that an an accelerated frame of reference. That is how I understand the equivalene principle. Another way of saying this is that if they were identical infinetesimally, they would integrate identically, resulting in identical motions wrt to the accelerating lab frames. But then, we know that the motions are distinguishable experimentally. Not arguing with you on this because you are right. I have taken this to mean that there is a fundamental difference between the motions of the objects and the frames. In fact, it would seem, physically, that they are precisely the opposite of each other, a mirror image so to speak. Welcome any and all comments. I don't see how you can conclude there is a difference between the object's motion and the object's frame of reference. In re-reading what I posted, I can understand the confusion you are having with what I said. I meant something entirely different than what you inferred. I'll try to do a better job. The the "inertial" objects are "all moving inertially wrt each other" and "accelerating identically" wrt to the accelerating lab far from a gravity source. While in the accelerating lab resting on the surface of the planet, the "inertial objects are all "accelerating with respect to each other" and "accelerating differently" wrt the lab frame. Physically, they seem to be opposites, that is, in terms of the qualities of their necessary motions. Is this clearer? Perfectly. Phil |
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#10
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Pete wrote: Try reading this. http://xxx.lanl.gov/abs/physics/0204044 It is a paper I wrote a few years back. The intent of the paper is to directly answer your question. Your historical account on the development of GR is very incomplete and misleading. We all know how Newton devised the law of gravity by watching a falling apple under gravitational influence. Einstein's breakthrough tried to outdo Newton by fantasizing himself as that apple falling under the influence of gravity. Hey, as doctor Roberts ingeniously pointed out. The outcome of that would eventually intercept the ground in a tragic end. So, Einstein co-operated with Grossmann trying to devise a theory of gravity based on his version of Equivalence Principle. It turned out to be a failure. Disgusted with Grossmann, he started looking for help in Goettingen. At Goettingen, Klein, Hilbert, and Schwarzschild were very good friends with Minkowski who had since passed away but not before suggesting the postulate on the existence of spacetime after abandoning the Aether by the scientific communities. Thus, Hilbert was interested in Einstein's work. However, instead of co-operation, Einstein and Hilbert became rivals with each one trying to beat the other one in coming up with the field equations. A spark came to Hilbert after Einstein bragged about derivation of Mercury's orbital anomaly. This derivation without using GR and thus without the necessary Schwarzschild metric was an entire plagiarism of Gerber's work. Of course, Hilbert did not know Einstein's work was total BS. Thinking he had lost the race, he basically pulled out a Hail-Mary throw. He pulled out this Hilbert Langrangian out of his *ss, and the field equations were born. Thus, GR was actually Hilbert's work. Somehow, you have just blacked out this part of the history, is it because you don't understand the field equations? |
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