Effective Potential for Even-Parity Regge-Wheeler Gravitational Perturbation Equations
Frank J. ZerilliPhysics Department, University of North Carolina, Chapel Hill, North Carolina 27514
1970en
ABI
Abstract
The Schr\"odinger-type equation for odd-parity perturbations on a background geometry has been extended to the even-parity perturbations. This should greatly simplify the analysis for calculations of gravitational radiation from stars and from objects falling into black holes.
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Cited by 90 references