Calculating Gravitational Radiation from Collisions

Details Calculating Gravitational Radiation from Collisions Calculating Gravitational Radiation from Collisions

2000-11-29

arxiv.org/abs/gr-qc/0011109v1

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

9 pages; to be published in the proceedings of the Conference on Stellar Collisions (American Museum of Natural History, June

Scientific paper

The development of both ground- and space-based gravitational wave detectors provides new opportunities to observe the radiation from binaries containing neutron stars and black holes. Numerical simulations in 3-D are essential for calculating the coalescence waveforms, and comprise some of the most challenging problems in astrophysics today. This article briefly reviews the current status of efforts to calculate black hole and neutron star coalescences, and highlights challenges for the future.

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