Rarita-Schwinger fields in the Kerr geometry

Details Rarita-Schwinger fields in the Kerr geometry Rarita-Schwinger fields in the Kerr geometry

Dec 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990phrvd..42.4082d&link_type=abstract

Physical Review D, vol. 42, Issue 12, pp. 4082-4086

Physics

6

Scientific paper

The spin-3/2 perturbations of a rotating black hole are analyzed in the framework of linearized supergravity, expressing the complete solution of the Rarita-Schwinger equation in terms of a Debye potential. The equation governing the Debye potential is separated and the radial equation is transformed into a Schrödinger-type equation with a short-range potential from which the reflection and transmission coefficients can be calculated.

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