Gravitational Radiation Damping
- 29 July 1968
- journal article
- research article
- Published by American Physical Society (APS) in Physical Review Letters
- Vol. 21 (5) , 320-323
- https://doi.org/10.1103/physrevlett.21.320
Abstract
An analysis is presented of the emission of gravitational waves by a star in nonradial pulsation. This analysis, rigorous to first order in the pulsation amplitude and to all orders in and , exhibits damping of the pulsation as the waves are emitted (gravitational radiation reaction).
Keywords
This publication has 9 references indexed in Scilit:
- Erratum: Non-Radial Pulsation of General-Relativistivc Stellar Models. I. Analytic Analysis for L ≥ 2The Astrophysical Journal, 1968
- Gravitational Radiation in the Limit of High Frequency. II. Nonlinear Terms and the Effective Stress TensorPhysical Review B, 1968
- Non-Radial Pulsation of General-Relativistic Stellar Models. I. Analytic Analysis for L ≥ 2The Astrophysical Journal, 1967
- Superdense StarsAnnual Review of Astronomy and Astrophysics, 1966
- The equations of motion of slowly moving particles in the general theory of relativityIl Nuovo Cimento (1869-1876), 1965
- The EIH equations of motion up to the 9th orderPhysics Letters, 1964
- Lorentz-Invariant Equations of Motion of Point Masses in the General Theory of RelativityPhysical Review B, 1962
- Gravitational motion and radiation — IIIl Nuovo Cimento (1869-1876), 1959
- Radiation Damping in General RelativityPhysical Review B, 1957