Gravitational radiation from rotating gravitational collapse

Astronomy and Astrophysics – Astronomy

Scientific paper

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Black Holes (Astronomy), Gravitational Collapse, Gravitational Waves, Relativity, Computer Programs, Hydrodynamic Equations, Pattern Recognition, Signatures, Stellar Rotation, Waveforms

Scientific paper

The efficiency of gravitational wave emission from axisymmetric rotating collapse to a black hole was found to be very low: Delta E/Mc sq. less than 7 x 10-4. The main waveform shape is well defined and nearly independent of the details of the collapse. Such a signature will allow pattern recognition techniques to be used when searching experimental data. These results (which can be scaled in mass) were obtained using a fully general relativistic computer code that evolves rotating axisymmetric configurations and directly computes their gravitational radiation emission.

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