Gravitational radiation from rotating gravitational collapse

Details Gravitational radiation from rotating gravitational collapse Gravitational radiation from rotating gravitational collapse

Aug 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989nascp3046...18s&link_type=abstract

In NASA, Relativistic Gravitational Experiments in Space p 18-24 (SEE N90-19940 12-90)

Astronomy and Astrophysics

Astronomy

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.

Affiliated with

Also associated with

No associations

Rating

Gravitational radiation from rotating gravitational collapse does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Gravitational radiation from rotating gravitational collapse, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Gravitational radiation from rotating gravitational collapse will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1519645