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Black Holes - the two points of view. |
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| Aug27-12, 09:48 PM | #69 |
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Black Holes - the two points of view.It is not true that mass makes no difference under this scheme. Stress-energy and geometry are interlinked, and parallel transport is affected by geometry (as are the way null paths connect world lines in Dalespam's approach). It is just that there is no need to factor it into separate effects, and in the general case, you can't. Synge's position was that the spacetime was either curved or not, period. And that the difference is detectable mathematically in an arbitrarily small region; in the limit at a single point. Therefore he felt it was simply false to say gravity and acceleration in flat spacetime were locally equivalent. I don't agree this makes the principle useless - it just defines the bounds of its accuracy. |
| Aug27-12, 11:40 PM | #70 |
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Given static observers S1, S2 with S2at infinity and free falling observer FF with rel velocity v wrt S2 S1 and FF emit identical signals at the moment of co-location. As received at S2 the signal from FF will be equivalent to the signal from S1 with the addition of a purely classical Doppler shift for relative velocity v. Is this right? If we consider another inertial frame I ,in flat spacetime with the same v relative to S2 would there be any difference in received signals at S2, between those from FF and I ??? Thanks for your patience |
| Aug28-12, 12:29 AM | #71 |
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So the answer is yes, though I'd reverse the order from your original phrasing, because the velocity between FF and S1 is well defined as they are at the same spot, and that way you don't have to worry about multiplication being commutative (though it is). |
| Aug28-12, 03:04 AM | #72 |
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In your case there would only be transverse Doppler between FF and S 1 so there would not be any classical kinematic component ,only a simple gamma dilation factor. But from your input it appears I was wrong in my first conclusion. It seems you are saying there are two effects in operation. So a direct signal from FF to S2 would be red shifted by the full relativistic Doppler factor (which includes a gamma dilation component) and the additional gravitational dilation factor due to potential location. Do I have it yet?? Thanks |
| Aug28-12, 06:40 AM | #73 |
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I am imagining that FF is falling into the black hole, so that FF, S1, and S2 will always be in a straight line. I don't think it necessarily matters if they aren't, but I'll agree it's not as obvious if S1 doesn't automatically "intercept" the signal from FF "en-route" to S2. |
| Aug28-12, 07:03 AM | #74 |
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| Aug28-12, 07:14 AM | #75 |
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Mentor
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| Aug28-12, 07:39 AM | #76 |
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So FF is falling by S1 and emits the photon in passing. [QUOTE=Austin0;4050761] And no moving away from S1,,, a single transmission, ___SO if you might reread my previous post and see if it now tracks. Thanks_______________ |
| Aug28-12, 07:48 AM | #77 |
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Mentor
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| Aug28-12, 03:46 PM | #78 |
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Basically in practice you have to assume validity of the Hubble parameter to calculate a coordinate velocity of the emitter and obtain the redshift. |
| Aug28-12, 03:54 PM | #79 |
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"parallel transport the 4 velocity of the emitter at moment of emission, along the null path the light follows to the receiver, then apply SR doppler formula using the transported emitter 4-velocity expressed in the local frame of the receiver, and the null path tangent also expressed in this local receiver frame" It is a complete, unambiguous prescription, which Synge showed to always yield the correct result. |
| Aug28-12, 07:00 PM | #80 |
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The null geodesic approach is a good one, I don't mean to imply by discussing other approaches that its not.
Do note that if you have multiple images, you can in general have a different doppler shift for each image - so it doesn't necessarily solve the path dependence problems. |
| Aug28-12, 07:08 PM | #81 |
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Thus, Synge's (and Dalespam's equivalent) approach handle this case naturally: For each image, you use the the corresponding null path. I don't know what other approach you can use for this case. In any case, the following wording was misleading: "a unique transport path is specified, with a unique result" You don't have to worry about all paths, but you do have to worry about all null paths light actually follows, and compute a separate redshift for each. |
| Aug28-12, 07:34 PM | #82 |
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I haven't posted here for a few days, as I have had a lot to think about, but I have found your conversatiion interesting, and I am learning all the time.
I realise now that I was wrong about redshifts. There are what I think of as two processes, gravitational redshift and Doppler redshift, though some of you say it is all the same process. But I had thought there was an additionaln redshift because successive light signals from the falling body take longer and longer to escape the gravitation well. I see now that as I am thinking about separate signals at fixed intervals, this does not appear as a redshift, although it will add an added apparent time dilation as seen by a stationary distant observer. Have been reading up on naked singularities, and am about to email Saul Teukolsky to get more info from the horse's mouth. We got our B.Sc.s at the University of the Witwatersrand, but different generations. Mike |
| Aug29-12, 05:38 AM | #83 |
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As you admit below path dependence is not removed, so I won't enter into that issue. I'm not saying Synge (and Hogg and Bunn) "prescription" is wrong, I think it is purely an interpretational(almost just about terminology) issue, no matter how you call it (Doppler or cosmological redshift) the result must be the same, and yes, it can be computed in one step. |
| Aug29-12, 07:41 AM | #84 |
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| Aug29-12, 08:43 AM | #85 |
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For some reason you seem to avoid admitting that. |
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