Post-Newtonian Gravitational Radiation from Point Masses in a Hyperbolic Kepler Orbit

R. O. Hansen
Phys. Rev. D 5, 1021 – Published 15 February 1972
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Abstract

The energy and the angular momentum radiated away in the form of gravitational waves from a system of two point particles with positive total energy are calculated in the lowest nonvanishing post-Newtonian approximation. By these radiations a particle arriving from infinity can be captured, and the cross section for such captures is determined as a function of the energy at infinity. The radiation from elliptic (bound) orbits can also be inferred, and is found to be in agreement with known results.

  • Received 18 August 1971

DOI:https://doi.org/10.1103/PhysRevD.5.1021

©1972 American Physical Society

Authors & Affiliations

R. O. Hansen

  • University of Chicago, Chicago, Illinois 60637

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Issue

Vol. 5, Iss. 4 — 15 February 1972

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