The generation of gravitational waves. III - Derivation of bremsstrahlung formulae

Details The generation of gravitational waves. III - Derivation of bremsstrahlung formulae The generation of gravitational waves. III - Derivation of bremsstrahlung formulae

Oct 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977apj...217..252k&link_type=abstract

Astrophysical Journal, Part 1, vol. 217, Oct. 1, 1977, p. 252-280.

Physics

19

Bremsstrahlung, Celestial Mechanics, Collision Parameters, Field Theory (Physics), Gravitational Waves, Stellar Motions, Gravitational Fields, Integral Equations, Radiation Distribution, Relativistic Velocity, Space-Time Functions, Tensor Analysis, Trajectory Analysis

Scientific paper

Formulas are derived describing the gravitational waves produced by a stellar encounter of the following type. The two stars have stationary (i.e., nonpulsating) nearly Newtonian structures with arbitrary relative masses; they fly past each other with an arbitrary relative velocity; and their impact parameter is sufficiently large that they gravitationally deflect each other through an angle that is small as compared with 90 deg.

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