Gravitational radiation quadrupole formula is valid for gravitationally interacting systems

Details Gravitational radiation quadrupole formula is valid for gravitationally interacting systems Gravitational radiation quadrupole formula is valid for gravitationally interacting systems

Dec 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980phrvl..45.1741w&link_type=abstract

Physical Review Letters, vol. 45, Dec. 1, 1980, p. 1741-1744.

Physics

33

Gravitation Theory, Gravitational Fields, Quadrupoles, Stellar Gravitation, Stellar Systems, Two Body Problem, Binary Stars, Newton Theory, Space-Time Functions, Stress Tensors

Scientific paper

An argument is presented for the validity of the quadrupole formula for gravitational radiation energy loss in the far field of nearly Newtonian (e.g., binary stellar) systems. This argument differs from earlier ones in that it determines beforehand the formal accuracy of approximation required to describe gravitationally self-interacting systems, uses the corresponding approximate equation of motion explicitly, and evaluates the appropriate asymptotic quantities by matching along the correct space-time light cones.

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