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