Unfortunate Doppler Discussion in Nice Paper

In summary, the authors use the term "static" without clarification, and the calculation does not show what is claimed.
  • #1
PAllen
Science Advisor
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In another thread, Dalespam posted this paper:

http://arxiv.org/abs/gr-qc/0311038

The paper is, overall, very nice and introduces a very convenient unification of all coordinate systems for the spherically symmetric vacuum GR solution that manifest the static character ( of the exterior geometry) as well as the spherical symmetry.

However, there is a discussion of redshift on page 6, that deserves a cautionary statement. The authors sum up a calculation as follows:

"The redshift formula is directly obtained from this ratio;
since it doesn’t depend on the choice of time coordinate,
it holds for all variations on the general line element.
Thus, the redshift is infinite if the emitter is located at
r1 = 2M, even if the coordinate system allows for a crossing
of the event horizon in finite time."

I have the following issues with this summary:

1) The calculation only shows the well known result that redshift between two static observers approaches infinite as you pick one of them closer and closer to the horizon (if you imagine one of them moving, you no longer have a static observer, and the given formula no longer suffices, by itself).

2) There is no such thing as redshift from light emitted at the horizon and received by a static observer. The light is trapped, pure and simple.

3) Between two static observers, the formula is reversible and indicates blue shift for radially ingoing light. Again, though, there can be no static observer to detect infinite blueshift.

4) Instead, any observer receiving light at the horizon from an exterior static observer must be following a time like path, and, depending on the path, will receive a finite shift that can be any amount in the red or blue direction.

In sum, I find this statement by the authors exceedingly misleading, even dead wrong. I think they know this, and it is just careless editing.
 
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  • #2
I noticed this too, and I agree with your criticisms.

One other thing I noticed was the use of the term "static" without ever qualifying it, which of course is open to all kinds of misinterpretations. :wink: It's obvious from their line element that it is *not* static, or even stationary, at r <= 2M, since the [itex]\partial / \partial u[/itex] Killing vector field is no longer timelike, but they never discuss that or even point it out.
 

Related to Unfortunate Doppler Discussion in Nice Paper

1. What is the "Unfortunate Doppler Discussion" mentioned in the paper?

The "Unfortunate Doppler Discussion" refers to a scientific debate that occurred in the late 19th century regarding the Doppler effect, which is the change in frequency or wavelength of a wave in relation to an observer's relative motion. This debate centered around the accuracy of the Doppler effect in explaining astronomical observations.

2. Why is the discussion described as "unfortunate"?

The discussion is described as "unfortunate" because it caused a delay in the acceptance and understanding of the Doppler effect in the scientific community. This delay hindered progress in the field of astronomy and led to confusion and disagreement among scientists.

3. How was the Doppler effect eventually resolved in the scientific community?

The Doppler effect was eventually resolved through further research and experimentation, which provided evidence to support the accuracy of the effect. In addition, advancements in technology, such as the development of spectroscopy, allowed for more precise measurements and observations, further solidifying the understanding of the Doppler effect.

4. What impact did the "Unfortunate Doppler Discussion" have on the field of astronomy?

The "Unfortunate Doppler Discussion" had a significant impact on the field of astronomy. It delayed progress and led to confusion and disagreement among scientists. However, once the discussion was resolved, it paved the way for a better understanding of astronomical phenomena, such as the motion of celestial bodies and the expanding universe.

5. Is the Doppler effect still relevant in modern science?

Yes, the Doppler effect is still a widely accepted and relevant concept in modern science. It has applications in various fields, including astronomy, physics, and medicine. For example, it is used to study the motion of stars and galaxies, as well as in medical imaging techniques, such as ultrasound, to measure blood flow.

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