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Electromagnetic Waves in the Exterior of a Schwarzschild Black Hole
Published online by Cambridge University Press: 07 February 2017
Abstract
Using the technique of Debye potentials, the regular (nonstatic) EM fields are found to behave at r = M either as purely ingoing or as purely outgoing waves. After separation the radial equation is treated in the short wavelength approximation.
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- Part II: Stability and Collapse
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- Copyright © Reidel 1974