Abstract
The analytical solutions reported in our previous paper are given as series
of hypergeometric or Coulomb wave functions. By using them, we can get the
Teukolsky functions analytically in a desired accuracy. For the computation,
the deep understanding of their properties is necessary. We summarize the main
result: The relative normalization between the solutions with a spin weight s
and -s is given analytically by using the Teukolsky-Starobinsky (T-S)
identities. By examining the asymptotic behaviors of our solution and combined
with the T-S identities and the Wronskian, we found nontrivial identities
between the sums of coefficients of the series. These identities will serve to
make various expression in simpler forms and also become a powerful tool to
test the accuracy of the computation. As an application, we investigated the
absorption rate and the evaporation rate of black hole and obtain interesting
analytic results.
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