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limit of Rindler coordinates |
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| Nov30-12, 12:12 PM | #18 |
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limit of Rindler coordinateshttp://dx.doi.org/10.1007/BF02450447 "Covariance, invariance, and equivalence: A viewpoint" But how small is "small enough?" I think it's sufficient to say that it works in the limit as the box size approaches zero. The remark about the "orders" is simply a helpful way to help understand why the equivalence is exact in the limit, and non-exact over larger regions. It was not my intention to represet is aspart of any formal statement or defintion of the equivalence principle. Other proferred statements of the equivalence principle as "The Universality of Free Fall" seem to me to be clearer formulation of the equivalence principle than the original formulation about trying to determine whether or not you're in an elevator or on a planet by the means of physical experiments - as there are known means of building reasonably compact gravity gradient meters (such as the Forward mass detector, variants of which are actually used in prospecting for oil) [add] Another reference: http://dx.doi.org/10.1007/BF00763538 |
| Nov30-12, 12:39 PM | #19 |
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| Nov30-12, 05:58 PM | #20 |
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Meanwhile, there's an interesting paper I ran across (it may disappear from public access today) that takes a different position on the equivalence principle that may be helpful. Gravitational redshift and the equivalence principle The thing that is prescribed directly is that "the field must be uniform. This means no differences in the accelerometer readings between h and h+dh. This rules out tidal forces. THis is similar to the earlier observation I made that for small enough "h", there isn't any difference between the gravitational field due to the acceleration and the gravitational field due to matter - the time dilation is (1+/-gh) in each case. BTW, this is one of the relations that this paper derives with an effort to be exact and not make approximations. The authors don't directly prescribe that there is no matter in the "accelerated spacetime", and I suppose as long as the first condition is met, it's not necessary. You simply have a hybrid case, where you have gravitation due to matter plus gravitation due to acceleration, and they both follow the EP (as long as you don't choose a region so big that g varies over the region). However, the authors make a point of analyzing the case where there is no matter present, even though they don't prescribe it as "necessary". |
| Dec1-12, 01:02 AM | #21 |
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Do MTW give definition of "uniform gravitational field" in their book? Or rather do they explain how "uniform gravitational field" is related to "gravitational field"? I believe that they don't and in that case this formulation is useless. And where did you get your definition of "uniform gravitational field"? I believe that in order to get rid of tidal forces accelerometer readings should change according to particular law. If you take limit where we can't distinguish between different change rates in accelerometer readings then we can't talk about tidal forces (we can't distinguish between different levels of tidal forces) but we can't talk about equivalence with uniform acceleration either (equivalence becomes trivial). |
| Dec1-12, 01:32 AM | #22 |
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There is lengthy discussion about "uniform gravitational field" - http://www.physicsforums.com/showthread.php?t=156168
Hmm, is it possible to draw some conclusions from this discussion? |
| Dec1-12, 03:05 AM | #23 |
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| Dec1-12, 05:04 AM | #24 |
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From post #66 by Boustrophedon (and elaborated in #110), I think that Einstein's 1935 formulation (of which I gave an abbreviated version) is exact: a uniformly accelerated reference system (thus not "Born rigid") has accelerometers measuring the same "g" value everywhere; and that is postulated to be indistinguishable from a homogeneous gravitational field. Note that the EEP is non-local: Einstein admitted that it does not represent the whole Minkowski space; I suppose that he had something similar as Rindler's horizon in mind (but not exactly, as I first thought). |
| Dec1-12, 05:24 AM | #25 |
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While Einstein was a great man, physics didn't stop evolving with him. Elevating him to a cult personality figure isn't really the goal of physics. |
| Dec1-12, 05:28 AM | #26 |
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[edit] While I think the disussio has demonstrated that you can tell, it may not have gotten into great detail on the process of how you tell, But you yourself noticed the lack of freedom in the accelereometer readings for the acclerated observer. It's reasonably obvious I think that anything that deviates from this fixed profile can't be due to acceleration. It's probalby less obvious that if it does follow the profile, it is due to acceleration, but I think at least one of the papers goes into that calculation. |
| Dec1-12, 05:31 AM | #27 |
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| Dec1-12, 10:06 AM | #28 |
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| Dec1-12, 01:00 PM | #29 |
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| Dec1-12, 03:24 PM | #30 |
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Because nothing is varying with time, (physically or with the metric coefficients) it's not clear that there's any reason to limit the size of the box in the time direction. There are spatial variations in the field and the metric though (especially in the case of matter). Therefore we need to restrict the spatial size of the box if we want to avoid these variations (and it turns out we not only want to, but that we need to). Thus, while it's true that the acceleration is second order in time, it's not relevant to the point that the EP is trying to be made. There exists a set of cirumstances where the observation time is long enough that you can observe acceleration, but the tidal forces can be neglected, and in this set of circumstances, one can apply the equivalence principle. |
| Dec1-12, 05:37 PM | #31 |
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| Dec1-12, 05:39 PM | #32 |
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| Dec2-12, 01:12 AM | #33 |
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| Dec2-12, 01:53 AM | #34 |
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Acceleration on the other hand we view as intrinsic property of worldline, right? If I pick a single worldline one of it's properties is acceleration and we can somehow determine it without looking at context. Where tidal acceleration would require many worldlines. |
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