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The massive dirac equation in Kerr Geometry: Separability in Eddington-Finkelstein-type coordinates and asymptotics

URN to cite this document:
Röken, Christian
Date of publication of this fulltext: 17 Dec 2015 12:50


The separability of the massive Dirac equation in a rotating Kerr black hole background in horizon-penetrating advanced Eddington-Finkelstein-type coordinates is shown. To this end, the Kerr spacetime is described in the framework of the Newman-Penrose formalism by a local Carter tetrad, and the Dirac wave functions are given on a spin bundle in a chiral Newman-Penrose dyad representation. ...


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