Peeling for tensorial wave equations on Schwarzschild spacetime
arXiv:2206.02193 · doi:10.1142/S0129055X2350023X
Abstract
In this paper, we establish the asymptotic behaviour along outgoing and incoming radial geodesics, i.e., the peeling property for the tensorial Fackrell-Ipser and spin Teukolsky equations on Schwarzschild spacetime. Our method combines a conformal compactification with vector field techniques to prove the two-side estimates of the energies of tensorial fields through the future and past null infinity and the initial Cauchy hypersurface in a neighbourhood of spacelike infinity far away from the horizon and future timelike infinity. Our results obtain the optimal initial data which guarantees the peeling at all orders.
22 pages
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