Summary
The relations between the gravitational and electromagnetic perturbation functions of Zerilli and those of Lee in the Newman-Penrose formalism are explicitly derived.
Riassunto
Si derivano in forma esplicita le relazioni tra funzioni di perturbazione gravitazionali ed elettromagnetiche di Zerilli e quelle di Lee nel formalismo di Newman-Penrose.
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References
F. Zerilli:Phys. Rev. D,9, 860 (1974).
M. Johnson, R. Ruffini andF. Zerilli:Phys. Rev. Lett.,31, 1317 (1973).
V. Moncrief:Phys. Rev. D,9, 2707 (1974);10, 1057 (1974);12, 1526 (1975).
D. Chitre:Phys. Rev. D,13, 2713 (1976).
C. Lee:Journ. Math. Phys.,17, 1226 (1976).
C. Lee:Nuovo Cimento,41 B, 305 (1977).
One complex parameter (or two real parameters) is needed to fix the magnitude and the phase of each of the eight possible polarizations.
E. Newman andR. Penrose:Journ. Math. Phys.,3, 566 (1962).
S. Bose:Journ. Math. Phys.,16, 772 (1975).
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Lee, C.H. Study on perturbations in the Reissner-Nordström background geometry. Nuov Cim B 44, 123–134 (1978). https://doi.org/10.1007/BF02730335
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DOI: https://doi.org/10.1007/BF02730335