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  The close limit from a null point of view: The advanced solution

Campanelli, M., Gomez, R., Husa, S., Winicour, J., & Zlochower, Y. (2001). The close limit from a null point of view: The advanced solution. Physical Review D, 63(12): 124013.

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Item Permalink: http://hdl.handle.net/11858/00-001M-0000-0013-5591-F Version Permalink: http://hdl.handle.net/11858/00-001M-0000-0013-5593-B
Genre: Journal Article

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3365.pdf (Preprint), 566KB
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 Creators:
Campanelli, Manuela1, Author
Gomez, Roberto, Author
Husa, Sascha1, Author              
Winicour, Jeffrey1, Author
Zlochower, Yosef, Author
Affiliations:
1Astrophysical Relativity, AEI-Golm, MPI for Gravitational Physics, Max Planck Society, escidoc:24013              

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 Abstract: We present a characteristic algorithm for computing the perturbation of a Schwarzschild spacetime by means of solving the Teukolsky equation. We implement the algorithm as a characteristic evolution code and apply it to compute the advanced solution to a black hole collision in the close approximation. The code successfully tracks the initial burst and quasinormal decay of a black hole perturbation through 10 orders of magnitude and tracks the final power law decay through an additional 6 orders of magnitude. Determination of the advanced solution, in which ingoing radiation is absorbed by the black hole but no outgoing radiation is emitted, is the first stage of a two stage approach to determining the retarded solution, which provides the close approximation waveform with the physically appropriate boundary condition of no ingoing radiation.

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Language(s): eng - English
 Dates: 2001-06-15
 Publication Status: Published in print
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 Identifiers: eDoc: 3365
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Title: Physical Review D
Source Genre: Journal
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Pages: - Volume / Issue: 63 (12) Sequence Number: 124013 Start / End Page: - Identifier: -