COLLISION OF HIGHLY RELATIVISTIC PARTICLES WITH BLACK HOLES: THE GRAVITATIONAL RADIATION GENERATED

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ID: 271281
2003
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Abstract
We consider the high-speed collision of a particle with a black hole, and compute the gravitational wave spectra and total radiated energy, for both rotating and non-rotating holes. Some interesting properties of the energy spectrum characterize these processes, such as universal zero frequency limit and a power-law dependence on the multipole index. Making the extrapolation to the two black hole collision at the speed of light case, we conclude that this is the most efficient gravitational wave generator in the Universe.
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Authors Vitor Cardoso,José P. S. Lemos,Alexander Krasnitz,Robertus Potting,Ana M Mourão,Mário Pimenta;Vitor Cardoso;José P. S. Lemos;Alexander Krasnitz;Robertus Potting;Ana M Mourão;Mário Pimenta;
Journal The Identification of Dark Matter
Year 2003
DOI
10.1142/9789812791160_0024
URL
https://sciprofiles.com/publication/view/1023a8f2ec98bb2e194e0b3b438dde83
Keywords
frequency speed black hole spectra efficient gravitational multipole rotating

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