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

30 March 1970

journal article
research article
Published by American Physical Society (APS) in Physical Review Letters

Vol. 24 (13) , 737-738
https://doi.org/10.1103/physrevlett.24.737

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.

Keywords

PARITY PERTURBATIONS
PERTURBATION EQUATIONS
ODD PARITY
PARITY REGGE
GRAVITATIONAL RADIATION
OBJECTS FALLING
BLACK HOLES

This publication has 3 references indexed in Scilit:

Non-Radial Pulsation of General-Relativistic Stellar Models. II. Properties of the Gravitational Waves
The Astrophysical Journal, 1969
Non-Radial Pulsation of General-Relativistic Stellar Models. I. Analytic Analysis for L ≥ 2
The Astrophysical Journal, 1967
Stability of a Schwarzschild Singularity
Physical Review B, 1957