Relativistic longitudinal Doppler effect Relativistic Doppler shift for the longitudinal case, with source and receiver moving directly towards or away from each other, is often derived as if it were the classical phenomenon, but modified by the addition of a
time dilation term. This is the approach employed in first-year physics or mechanics textbooks such as those by Feynman or Morin. The transverse Doppler effect is one of the main novel predictions of the special theory of relativity. Whether a scientific report describes TDE as being a redshift or blueshift depends on the particulars of the experimental arrangement being related. For example, Einstein's original description of the TDE in 1907 described an experimenter looking at the center (nearest point) of a beam of "
canal rays" (a beam of positive ions that is created by certain types of gas-discharge tubes). According to special relativity, the moving ions' emitted frequency would be reduced by the Lorentz factor, so that the received frequency would be reduced (redshifted) by the same factor. On the other hand, Kündig (1963) described an experiment where a
Mössbauer absorber was spun in a rapid circular path around a central Mössbauer emitter. As explained below, this experimental arrangement resulted in Kündig's measurement of a blueshift.
Source and receiver are at their points of closest approach In this scenario, the point of closest approach is frame-independent and represents the moment where there is no change in distance versus time. Figure 2 demonstrates that the ease of analyzing this scenario depends on the frame in which it is analyzed.
One object in circular motion around the other Figure 5 illustrates two variants of this scenario. Both variants can be analyzed using simple time dilation arguments. The converse, however, is not true. The analysis of scenarios where
both objects are in accelerated motion requires a somewhat more sophisticated analysis. Not understanding this point has led to confusion and misunderstanding.
Source and receiver both in circular motion around a common center Suppose source and receiver are located on opposite ends of a spinning rotor, as illustrated in Figure 6. Kinematic arguments (special relativity) and arguments based on noting that there is no difference in potential between source and receiver in the pseudogravitational field of the rotor (general relativity) both lead to the conclusion that there should be no Doppler shift between source and receiver. In 1961, Champeney and
Moon conducted a
Mössbauer rotor experiment testing exactly this scenario, and found that the Mössbauer absorption process was unaffected by rotation. They concluded that their findings supported special relativity. This conclusion generated some controversy. A certain persistent critic of relativity maintained that, although the experiment was consistent with general relativity, it refuted special relativity, his point being that since the emitter and absorber were in uniform relative motion, special relativity demanded that a Doppler shift be observed. The fallacy with this critic's argument was, as demonstrated in section
Point of null frequency shift, that it is simply not true that a Doppler shift must always be observed between two frames in uniform relative motion. Furthermore, as demonstrated in section
Source and receiver are at their points of closest approach, the difficulty of analyzing a relativistic scenario often depends on the choice of reference frame. Attempting to analyze the scenario in the frame of the receiver involves much tedious algebra. It is much easier, almost trivial, to establish the lack of Doppler shift between emitter and absorber in the laboratory frame.
Motion in an arbitrary direction The analysis used in section
Relativistic longitudinal Doppler effect can be extended in a straightforward fashion to calculate the Doppler shift for the case where the inertial motions of the source and receiver are at any specified angle. Figure 7 presents the scenario from the frame of the receiver, with the source moving at speed v at an angle \theta_r measured in the frame of the receiver. The radial component of the source's motion along the line of sight is equal to v \cos{\theta_r}. The equation below can be interpreted as the classical Doppler shift for a stationary and moving source modified by the Lorentz factor \gamma : {{NumBlk|| f_r = \frac{f_s}{\gamma\left(1 + \beta \cos\theta_r\right)}.|}} In the case when \theta_r = 90^{\circ}, one obtains the
transverse Doppler effect: f_r = \frac {f_s} {\gamma}. In his 1905 paper on special relativity, In electromagnetic waves both the electric and the magnetic field amplitudes
E and
B transform in a similar manner as the frequency: \begin{align} E_r &= \gamma \left( 1 - \beta \cos \theta_s \right) E_s \\ B_r &= \gamma \left( 1 - \beta \cos \theta_s \right) B_s. \end{align} ==Visualization==