Wave Mechanics help-for optics course

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SUMMARY

The discussion focuses on deriving the radiation fields of an electrically charged particle attached to a vibrating string, described by the equation z(x, t) = z0sin((2*pi*n/L)x) cos(omega*t). Participants clarify the conversion of this equation into spherical coordinates and the subsequent application of the radiation field equations for electric and magnetic fields, specifically ERAD and BRAD. Key equations include the vector forms of the electric field ERAD and magnetic field BRAD, with emphasis on the use of spherical coordinates and unit vectors. The conversation highlights the importance of differentiating unit vectors and applying the BAC-CAB triple product rule in vector calculus.

PREREQUISITES
  • Understanding of wave mechanics and stationary vibration modes
  • Familiarity with spherical coordinates and vector calculus
  • Knowledge of electromagnetic radiation fields, specifically ERAD and BRAD
  • Proficiency in calculus, particularly differentiation of vector functions
NEXT STEPS
  • Study the derivation of electromagnetic radiation fields from moving charges
  • Learn about the BAC-CAB triple product rule in vector calculus
  • Explore the relationship between Cartesian and spherical coordinate systems
  • Review the principles of unit vectors and their applications in physics
USEFUL FOR

Students and professionals in physics, particularly those studying electromagnetism, wave mechanics, and vector calculus. This discussion is beneficial for anyone seeking to understand the derivation of radiation fields in the context of charged particles and vibrating systems.

  • #31


Im using the integral table laws of sins/cosines and for the integral of cos^2 I am using the integral of cos^2 = 1/2(x + sinxcosx)...after simplifying everything to what i believe is correct i end up with...

\frac{1}{2} (2\pi + sin(2\pi - \frac{\omega r}{c})cos(2\pi - \frac{\omega r}{c}) - sin(\frac{\omega r}{c})cos(\frac{\omega r}{c}))
 
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  • #32


Huh?! I've never seen that trig ID before (because it is incorrect). I've seen cos^2(x)=\frac{1}{2}(1-cos(2x) before though. There is an easier way though; the integral of cos^2 over a full period represents the area under cos^2 from 0 to T. Due to symmetry, the area under sin^2 will be the same so

\int_0^T cos^2(\omega(t-r/c))dt=\frac{1}{2} \left(\int_0^T cos^2(\omega(t-r/c))dt +\int_0^T sin^2(\omega(t-r/c))dt \right)

=\frac{1}{2} \int_0^T (cos^2(\omega(t-r/c)) + sin^2(\omega(t-r/c)))dt=\frac{1}{2} \int_0^T (1)dt=\frac{T}{2}

\Rightarrow \left< cos^2(\omega(t-r/c)) \right> _T=\frac{1}{2}

I think you are probably supposed to take a spatial average of P_rad as well, in that case, just integrate the r,theta and phi dependent terms over the volume of a sphere and divide by the volume.
 
  • #33


Thats because its not a trig identity, it was the integral, although i did it incorrectly anyway.

So the power simplified is..

\frac{q^2 \omega^4 z^2_0}{12\pi\epsilon_0 c^3} * sin^2(\frac{2\pi n}{L} rsin\theta cos\phi + a)

There is no mention of a spatial average in the hw, nor in my notes.
 
  • #34


Well, the question asks for the average energy per unit time. To me, that means spatial and temporal average. It makes no sense that the average power would depend on your position in the radiation field.
 
  • #35


I will ask the professor tomorrow what exactly he is looking for. The only thing i have in my notes for average power (that is the same as average energy per unit time right?) is:

power = \frac{q^2}{6\pi\epsilon c^3} *a(t-\frac{r}{c})

Looking over my notes I think we did do the spatial average during the derivation of the above formula...part the derivation consists of what you described on the previous page.

Then he gave us the average power formula

power = \frac{q^2}{6\pi\epsilon c^3} *<a(t-\frac{r}{c})>_T
 

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