Is the Transverse Doppler Effect Dependent on General Relativity?

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Discussion Overview

The discussion centers on the transverse Doppler effect and its dependence on special relativity versus general relativity, particularly in scenarios where the motion of the source is perpendicular to the observer's position vector. Participants explore the implications of non-uniform motion and the conditions under which the transverse Doppler effect is valid.

Discussion Character

  • Debate/contested
  • Technical explanation
  • Conceptual clarification

Main Points Raised

  • One participant questions whether the validity of the transverse Doppler effect relies on general relativity when the source rotates around the observer, suggesting that the source's non-uniform motion may necessitate a different treatment.
  • Another participant argues that the derivation of the transverse Doppler effect does not require pure transverse motion, asserting that as long as there is a transverse component, time dilation accounts for the effect, and special relativity suffices.
  • A later reply reiterates that the special relativistic formula for the transverse Doppler shift remains valid for an inertial observer, unless gravitational effects are considered, which would require general relativity.
  • One participant acknowledges understanding the derivation of the transverse Doppler effect from special relativity and clarifies that their concern is about the limiting case of motion when the radial component approaches zero, questioning the uniformity of motion in that scenario.

Areas of Agreement / Disagreement

Participants express differing views on whether the transverse Doppler effect's validity is contingent on general relativity or if special relativity is sufficient. The discussion remains unresolved, with multiple competing perspectives presented.

Contextual Notes

Participants note that the discussion involves assumptions about the nature of motion (uniform vs. non-uniform) and the potential influence of gravitational sources on the Doppler effect, which are not fully resolved.

arildno
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I saw in a chapter on special relativity a derivation of the transverse Doppler effect, which seemed okay, but I have a question concerning this:

If the motion of a source is always perpendicular to the position vector connecting the observer to the moving source (i.e. the distance remains constant), that is the source rotates about the obs., does not
(technically, at least) the validity of the result (transv. D. eff.) depend on general relativity, rather than special relativity, since the source's rest frame is in non-uniform motion relative to the observer's rest frame?
 
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As I am sure you realize, the derivation of the transverse Doppler effect does not require that the motion of the source be in pure transverse motion. As long as there is a transverse component of motion, there will be a transverse Doppler effect due to time dilation. In any case, even if the light source does purely circle around the observer, the observing frame is still inertial, so special relativity should be sufficient.

Or have I missed your point?
 
arildno said:
I saw in a chapter on special relativity a derivation of the transverse Doppler effect, which seemed okay, but I have a question concerning this:

If the motion of a source is always perpendicular to the position vector connecting the observer to the moving source (i.e. the distance remains constant), that is the source rotates about the obs., does not
(technically, at least) the validity of the result (transv. D. eff.) depend on general relativity, rather than special relativity, since the source's rest frame is in non-uniform motion relative to the observer's rest frame?

The special relativistic formula for transverse Doppler shift will still be valid for describing how the light is seen according to the inertial frame observer that was emmited from the circling object unless you are also considering a gravitational source such as a planet about which it orbits for example. Then, one must use general relativity to determine the total relativistic Doppler shift.
 
Thx for the response!
Doc Al, yes, I was aware of that the derivation of the transverse Doppler effect did not at all depend upon a pure transverse motion; in fact, the result followed from the decomposition of a uniform motion (in accordance with spec. rel.) into a radial and transverse component,
the radial comp. accounting for the classical Doppler effect, whereas the transverse effect enters as a result of the time dilation factor (since the transverse velocity component is part of the total velocity).

Hence, I have no trouble in recognizing the presence of a transverse Doppler effect in the case of a general, uniform motion, and that this is derivable from the postulates/conditions for the validity of special relativity.

My point only concerned the limiting case (radial comp->0),
i.e. when the motion can no longer be regarded as strictly uniform, since the source will, in fact, rotate around the observer.

However, from your own answer, and DW's, I think I have gained a satisfactory response.
 

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