1984
DOI: 10.1098/rspa.1984.0002
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On mass-dependent spheroidal harmonics of spin one-half

Abstract: The angular functions in Chandrasekhar’s separation of the variables of Dirac’s equation in Kerr geometry are solved by an expansion procedure based on spin-weighted spherical harmonics. The characteristic values are obtained as a series in a σ, where a is the Kerr parameter and σ is the frequency. Closed expressions are obtained for the successive terms in the expansion. Numerical tables are provided.

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Cited by 34 publications
(23 citation statements)
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“…In the 70's, and 80's we find a large number of publications regarding the angular equation Chakrabarti (1984), and Seidel (1989). According to these references we will also name the solution of the angular equation as spin-weighted spheroidal function (SWSF).…”
Section: Introductionmentioning
confidence: 99%
“…In the 70's, and 80's we find a large number of publications regarding the angular equation Chakrabarti (1984), and Seidel (1989). According to these references we will also name the solution of the angular equation as spin-weighted spheroidal function (SWSF).…”
Section: Introductionmentioning
confidence: 99%
“…For am = ±aω, the two canonical references on numerical approximations of λ n (κ; am, aω) are [8,10]. Suffern et al [8] derived an asymptotic expansion of the form…”
Section: Numerical Benchmarksmentioning
confidence: 99%
“…On the other hand, Chakrabarti [10] In both [8,10], the numerical estimation of λ n is achieved by means of a series expansions in terms of certain expressions involving aω and am, so it is to be expected that the approximations in both cases become less accurate as |aω| and |am| increase. However, no explicit error bounds are given in these papers and they seem to be quite difficult to derive.…”
Section: Numerical Benchmarksmentioning
confidence: 99%
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