Synchrotron Spectrum: Constructing an Emission Spectrum

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Discussion Overview

The discussion revolves around constructing the emission spectrum of a relativistic electron in a homogeneous magnetic field, specifically focusing on synchrotron radiation. Participants explore the derivation of intensity using the Doppler effect and the implications of Fourier transformation on the resulting spectrum.

Discussion Character

  • Technical explanation
  • Mathematical reasoning
  • Debate/contested

Main Points Raised

  • One participant describes deriving the emission spectrum using the invariance of intensity and frequency, applying the Doppler effect to relate the observed intensity to the emitted intensity.
  • Another participant points out that the initial spectrum represents intensity over time rather than the frequency of emitted radiation, suggesting the need for complex amplitude to accurately determine frequency peaks.
  • A participant questions the reliance on periodic motion for frequency dependence and proposes correcting the formula to include proper intensity in the rest frame to achieve a more accurate spectrum.
  • Another participant agrees that the frequency dependence of radiation emitted at a specific moment must be considered for accurate results.

Areas of Agreement / Disagreement

Participants express differing views on the adequacy of the initial formula used for intensity and the methods for deriving the correct emission spectrum. There is no consensus on the best approach to correct the spectrum or the implications of the Fourier transformation.

Contextual Notes

Participants note limitations in the initial approach regarding the frequency dependence and the need for a more nuanced understanding of the emitted radiation at specific moments in time. The discussion highlights unresolved mathematical steps and assumptions regarding the parameters involved.

lakmus
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Hi!
I try to construct the emission spectrum from relativistic electron rotating in homogeneous magnetic field - synchrotron. In my lecture notes a found out one really easy derivation using the invariance of
[itex]\frac{I'}{(\nu')^3}=\frac{I}{\nu^3}[/itex], where [itex]I[/itex] is the specific intensity and [itex]\nu[/itex] is
the frequency. So the radiated intensity from inertial observe frame is
[itex]I'=\frac{I (\nu')^3}{\nu^3}[/itex], using Doppler effect fromula
[itex]I'=\frac{I}{\gamma^3\left(1-\frac{v}{c}\cos{\theta}\right)^3}[/itex], where [itex]\theta[/itex] is angle possition on the circular trajectory. I used [itex]\theta = \frac{\omega_{cyclotron} t}{\gamma}[/itex] . Then I plotted the resulting
intensity, which looked ok (at least similar to some I found on the internet). I also did the Fourier transformation (picture uploded). But the critical frequency is too height, also the peaks are to widt - here (http://farside.ph.utexas.edu/teaching/em/lectures/node133.html) I found, that the maximum radiadion should be emmited at frequency [itex]\propto \gamma^2 \omega_{cyclotron}[/itex] , blue line at the picture.
Thanks a lot for each advice!
 

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Your first spectrum shows the intensity over time. The Fourier transformation of this shows the frequency of intensity peaks, but not the frequency of the radiation itself. To get this, you would need the complex amplitude in the first plot, and you don't get this with the simple formula you used.

If you want the frequency of the emitted radiation, I think you can neglect the overall motion of the electron around the circle and focus on the parts where you get the intensity peaks. This won't work with your formula for the total intensity, however.
 
Ok, thanks a lot! I thought that it is quite weird, that the frequency dependence came only from the periodic motion. So could I try to correct this formula by adding proper intensity I in the rest frame - the correct frequency dependence? (I tried to change some parameteres and if the period of peaks remain the same, but they would be thinner, I will get more shorter frequences - the correct spectrum)
 
Yes, you need the frequency dependence of the radiation emitted "at one point in time" in some way.
 

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