I have been trying to derive the Teukolsky equation via the Newman-Penrose formalism. I have derived the following formula (see Eq. (2.14) in Teukolsky's paper)
\begin{equation} (*) \left[(\Delta +3\gamma - \gamma^*+4\mu + \mu^*)(D+4\epsilon-\rho)-(\delta^*-\tau^*+\beta^*+3\alpha+4\pi)(\delta-\tau+4\beta)-3\psi_2\right]\psi_4 = 0. \end{equation}
The Greek letters (except for $\psi_4$) are all defined with respect to the Kerr background.
What I am struggling with is: deriving the actual wave equation (Eq. (4.7) in Teukolsky's paper) for $\psi_4$ using the Kinnersly tetrad (see Eq (4.4)-(4.6) in Teukolsky's paper) in Boyer-Lindquist coordinates, starting from Eq.(*). I am plugging in the defined values like $\Delta=l^{\mu}\partial_{\mu}$, etc. but I cannot recover Teukolsky's full equation: I have the wrong coefficients for the $\partial_{\theta}\psi_4$, $\partial_{\phi}\psi_4$, $\partial_r\psi_4$, and $\psi_4$ components.
I would greatly appreciate notes on deriving the Teukolsky equation, a link to a mathematica notebook, or a demonstration in someones answer on going from the Newman-Penrose Eq.(*) to the Teukolsky equation in Boyer-Lindquist coordinates.
NOTE
In case the links break: Teukolsky's paper refers to:
- Teukolsky, Saul A.; Astrophysical Journal, Vol. 185, pp. 635-648 (1973)
Newman-Penrose refers to
- Newman, Ezra and Penrose, Roger; Journal of Mathematical Physics, Volume 3, Issue 3, p.566-578