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We give an expansion of the solution of the evolution equation for the massless Dirac fields in the outer region of de Sitter-Reissner-Nordstr"om black hole in terms of resonances. By means of this method we describe the decay of local energy for compactly supported data. The proof uses the cut-off resolvent estimates for the semi-classical Schr"odinger operators from Bony and H"afner, 2008. The method extends to the Dirac operators on spherically symmetric asymptotically hyperbolic manifolds.

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