To solve Equation (174), we first note the following. Unless the value of is such that the denominator in the expression of or happens to vanish, or happens to vanish in the limit , we have , , and . Also, from the asymptotic behavior of the minimal solution as given by Equation (134), we have and for sufficiently large . Thus, except for exceptional cases mentioned above, the order of in increases as increases. That is, the series solution naturally gives the post-Minkowski expansion.
First, let us consider the case of for . It is easily seen that , , and for all . Therefore, we have for all .
On the other hand, for , the order of behaves irregularly for certain values of . For the moment, let us assume that . We see from Equations (124) that , , since . Then, Equation (174) implies . Using the expansion of given by Equation (110), we then find (i.e., there is no term of in ). With this estimate of , we see from Equation (128) that is justified if is of order unity or smaller.
The general behavior of the order of in for general values of is rather complicated. However, if we assume to be a non-integer and , and , it is relatively easily studied. With the assumption that , we find there are three exceptional cases:
These imply that , , and , respectively. To summarize, we have
The post-Minkowski expansion of homogeneous Teukolsky functions can be obtained with arbitrary accuracy by solving Equation (123) to a desired order, and by summing up the terms to a sufficiently large . The first few terms of the coefficients are explicitly given in . A calculation up to a much higher order in was performed in , in which the black hole absorption of gravitational waves was calculated to beyond the lowest order.
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