Integrate source terms for test EM field in Kerr spacetime

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SUMMARY

This discussion focuses on integrating source terms for the electromagnetic field in Kerr spacetime, specifically addressing the integral involving the source terms \(J_m\) and \(J_n\). The user provided equations and constants, including the Dirac delta function and Spin-Weighted Spherical harmonics, while referencing the article "Stationary electromagnetic fields around black holes. II." A Mathematica notebook was shared for calculations, highlighting that the integrated source term is cubic in \(r\), contrasting with the quadratic term presented in the referenced article. The user seeks feedback on improving their calculations.

PREREQUISITES
  • Understanding of Kerr spacetime and its properties
  • Familiarity with Spin-Weighted Spherical harmonics
  • Proficiency in Mathematica for computational tasks
  • Knowledge of electromagnetic field theory in general relativity
NEXT STEPS
  • Review the article "Stationary electromagnetic fields around black holes. II." for context
  • Explore advanced techniques in Mathematica for symbolic integration
  • Study the properties and applications of Spin-Weighted Spherical harmonics
  • Investigate the implications of cubic versus quadratic source terms in electromagnetic theory
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Researchers and students in theoretical physics, particularly those studying general relativity, black hole physics, and electromagnetic field theory. This discussion is also beneficial for anyone using Mathematica for complex calculations in these areas.

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Homework Statement
Calculate the source term ##^2J_{lm}## while knowing by integrating the known quantities.
Relevant Equations
$$ ^2J_{lm}(r) = \int_0^{2\pi} \int_0^\pi \frac{(r- i a \cos \theta)^2}{(r_+ - r_-)^2} \Sigma \ J_2 \;{}_{-1}\overline{Y}_{lm} \sin \theta d\theta d \phi$$
Hello, the Homework Statement is quite long, since it includes a lot of equations so I will rather post the as images as to prevent mistypes.

We need to find the integral
1696784403607.png

where
1696784412160.png

with

$$
J_m =(\sqrt{2}(r−ia\cos⁡θ))^{−1} i(r^2+a^2)\sin⁡(θ)j,
$$

$$
J_n = - \frac{a \Delta}{ 2 \Sigma} \sin(\theta )^2 j,
$$

$$
j = C \delta(r-r_0) \delta(\theta-\pi /2),
$$

where δ is the dirac delta function and with
$$
\Delta = r^2 - 2 M r + a^2
$$

$$
\Sigma = r^2 + a^2 \cos(\theta)^2
$$Finally ##(r_+,r_-,r_0,C,a,M)## are constant and ## {}_{-1}\overline{Y}_{l,m} = {}_{-1}\overline{Y}_{l,m}(\theta,\phi) ## are the Spin-Weighted Spherical harmonics.

We were also given the article Stationary electromagnetic fields around black holes. II. I understand that not everyone has access to it. But I've provided everything necessary here.

Since the calculation are very long I've prepared a Mathematica notebook. Which I've attached as pdf and is also (with working Mathematica notebook) at https://github.com/Zlabekma/homework.git).

Anyway, I don't finish the calculation there because my integrated source term is at least cubic in the variable ##r## but the one in the article is only quadratic in ##r##.
To be more specific in the article they state that ##{}^2J_{lm} \propto \Delta##
Comments on how to improve this post are very much appreciated. Thank you.
 

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For clarity I finished the calculation using rules for Spin-Weighted Spherical harmonics and corrected a typo. I've modified the notebook and the pdf. But the problem of course remains.
 

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