Effective Potential for Even-Parity Regge-Wheeler Gravitational Perturbation Equations

Frank J. Zerilli
Phys. Rev. Lett. 24, 737 – Published 30 March 1970
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Abstract

The Schrödinger-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.

  • Received 29 January 1970

DOI:https://doi.org/10.1103/PhysRevLett.24.737

©1970 American Physical Society

Authors & Affiliations

Frank J. Zerilli

  • Physics Department, University of North Carolina, Chapel Hill, North Carolina 27514

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Issue

Vol. 24, Iss. 13 — 30 March 1970

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