Modeling sources of gravitational radiation

Details Modeling sources of gravitational radiation Modeling sources of gravitational radiation

Mar 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983entr........28e&link_type=abstract

Energy and Technology Review, March 1983, p. 28-37.

Statistics

Computation

Computerized Simulation, Gravitational Waves, Relativistic Theory, Stellar Models, Wave Propagation, Computer Programs, Computer Techniques, Stellar Evolution

Scientific paper

A computer code which permits simulation of some improbable astrophysical events which result in gravity waves is discussed. The problem of the wave propagation is solved in numerical relativity on a computational grid with two spatial dimensions. Nonrotating, axially symmetric systems are assumed. The technique of solving the numerical relativity problem is sketched, describing the roles of the ten gravity fields in the procedure. An example whose result is qualitatively known is used to test the accuracy of the technique. The final integrated energy flux agrees with the initial configuration of mass-energy to within 0.7 percent.

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