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Do particles and objects trend toward 0 velocity. |
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| Aug26-12, 05:29 PM | #1 |
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Do particles and objects trend toward 0 velocity.
Light traveling long distances through the universe will red-shift due to cosmic expansion. Particles like electrons also have a wavelength described by the equation λ=h/ρ. If an electron were traveling through the universe undisturbed would it's wavelength also be stretched by cosmic expansion resulting the loss of momentum? If so, would the same logic also apply to macroscopic object meaning that over cosmic distances and time scales all objects would trend toward 0 velocity with respect to the Hubble flow?
In the early universe when "cosmic time scales and distances" were tiny, could this be the mechanism that selected 1 particular frame of reference that we now observe as being at rest with respect to the CMB? |
| Aug27-12, 12:19 AM | #2 |
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I think you are confusing classical waves with quantum particles. I also suspect you are imagining that someone standing close to an very red-shifted object sees that object as very red. |
| Aug27-12, 01:57 AM | #3 |
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Red shift in Hubble's Law is due to relative velocities of gallaxies, not directly due to expansion. Photon is emitted already red-shifted relative to us, not becoming more and more red-shifted as time goes on. So your analysis is flawed right there.
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| Aug27-12, 10:44 AM | #4 |
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Do particles and objects trend toward 0 velocity.'Expansion' and Hubble flow are a result of the FRW metric, in particular a(t), and 'Redshift' is a measured [and unambiguous] shift in received frequency versus emitted frequency. [But exactly what such a shift represents is subject to interpretation.] In other metrics [cosmological models] there may not be superluminal expansion. PeterDonis and Chalnoth have, I believe, agreed on this, from a Chalnoth post: Photons do not lose energy in expansion. [url] ttp://www.physics.uq.edu.au/downloa...iAm_Energy.pdf][/url Excellent discussion here: "Carried along by the Hubble flow" http://www.physicsforums.com/showthread.php?t=614297 Marcus: "expansion causes things to lose momentum relative to the CMB." So if you send a rocket off at .1c (relative to ancient light) it will eventually slow down (relative to ancient light)…. Expansion bleeds momentum from a flash of light as well. It keeps going the same speed but its wavelength lengthens, which means its momentum is drained also. My comment: from Tamara Davis: |
| Aug27-12, 11:18 AM | #5 |
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http://www.mso.anu.edu.au/~charley/p...DavisSciAm.pdf (Page 9, specifically) suggests that yours is a common misconception about the expansion of the universe. |
| Aug27-12, 11:59 PM | #6 |
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That would be p43.
Or, even, wikipedia: http://en.wikipedia.org/wiki/Hubble%...shift_velocity ... agrees well with the idea of a linear doppler shift due to relative motion of distance objects. However - I still think there are many possible confusions evident in the question to be able to answer clearly at this point. We need to hear back from OP before making too many assumptions. |
| Aug28-12, 12:35 AM | #7 |
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How do I explain this in simple terms? Well, lets say I put a whole bunch of equidistant observers between Earth and the distant galaxy. Lets say I ask them to measure the wavelength of a single pulse of light emitted at said galaxy towards earth as it passes them by. What will they observe? Well, naturally, each observer will report a more and more red-shifted beam as they get further from the galaxy and closer to Earth. Hey, that seems consistent with what that article says! But wait, why is this happening? Are we sure the light's wavelength actually changes? Each observer is located in different part of space separated by some distance. Due to expansion, all these observers are moving away from each other. Each observer's coordinate system is moving with respect to other observer's coordinate systems. When you go from one coordinate system to the other, where they are not at rest with respect to each other, you will end up with corresponding red/blue shifts. So the disagreement between observers is still accounted for by simple Doppler shift. What gives? Well, this is actually very interesting. Metric that allows for uniform expansion of space actually requires all points in space to be moving apart from each other. The red shift due to the metric is absolutely equivalent to Doppler shift due to resultant motion. And it would point to a major flaw in GR if this was not the case. Now here is the fine point which the author of the article doesn't appear to understand. Light's wavelength in any inertial frame does not change. It behaving otherwise would require light to age, which is impossible since light is massless. The apparent expansion of light as it travels arises from light's wavelength being measured in different coordinate systems at different points along the journey. The coordinate system in the right panel of that page is an accelerated one. Will light red/blue shift in an accelerated frame? Well, yeah. But let us take a frame of reference that is not accelerating. For example, I can take the reference frame tied to the galaxy itself. In that frame, light is never red shifted. (I am ignoring gravitational red shift here.) From that frame of reference, the wavelength does not change all the way until it reaches Earth, which appears to be moving away. On the other hand, I can consider Earth as my inertial coordinate system. In that coordinate system, light doesn't change wavelength throughout the journey either. No acceleration. But in that coordinate system, the galaxy is moving away, so light became red shifted when it was emitted. So again. Relative to us light got emitted already red shifted. It did not get red shifted in journey. If you are comfortable with tensor calculus required for General Relativity, I can show you derivation of this effects using an actual simple example of an expanding space-time metric. It's fairly straight forward, but you do need to have some rudimentary understanding of GR to follow. |
| Aug28-12, 05:49 AM | #8 |
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Starting with the premise that space expands, it seems inescapable that the wavelength of light should expand also. If the wavelength of a given photon is 1000 nm and the space it is in expands at a rate if 1/140% per million years then after 1 billion years it should have a wavelength of 1074 nm. The fact that it's moving is irrelevant since every nm of space that it moves through is expanding uniformly. K^2 (or anyone else who shares his view), where is this reasoning flawed?
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| Aug28-12, 05:53 AM | #9 |
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In that space isn't a fixed grid. If it was, you'd have a concept of absolute velocity. But velocity is relative. Wavelength of light is entirely determined by the observer. So talking about what happens to wavelength of light without establishing a coordinate system is silly.
The coordinate system in which wavelength is gradually expanding is an accelerated one. In an inertial frame, it is not changing. It's that simple. |
| Aug28-12, 03:32 PM | #10 |
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K^2 posts:
K^2: Would you quote what you believe is in error?? Such a discussion would likely be of benefit to Mrspeedy....maybe me too!! |
| Aug28-12, 07:07 PM | #11 |
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For cosmic scale problems I find it convenient to use a reference frame in which "at rest" means at rest with respect to the CMB. Since any 2 objects at rest with respect to the CMB will be accelerating away from each other this is 1 type of accelerating coordinate system. Please revisit the original question with the understanding that all measurements are relative to the CMB. |
| Aug29-12, 05:32 PM | #12 |
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Mr speedy: I continue to agree with your original premise....relative to the CMB...
A few descriptions from experts in these forums I saved to clarify several perspectives: PALLEN: "It's nature that is bizzare, not the physics." "We know much, we understand little." |
| Aug29-12, 05:49 PM | #13 |
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Mr speedy...I'd reply to K^2's post #3
CMB was at about 3,000K when emitted, is now about 2.7K.... |
| Aug30-12, 12:39 AM | #14 |
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You might be right, though. I'm still working through the math. I was trying to demonstrate how this works properly in GR setting, and I have hit a few snags. Time dependent metrics are a bit of a pain to work with. Once I've worked through them, I'll post the results either way. |
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