Published January 15, 1998
| Published + Submitted
Journal Article
Open
Waveform propagation in black hole spacetimes: Evaluating the quality of numerical solutions
Chicago
Abstract
We compute the propagation and scattering of linear gravitational waves off a Schwarzschild black hole using a numerical code which solves a generalization of the Zerilli equation to a three-dimensional Cartesian coordinate system. Since the solution to this problem is well understood it represents a very good testbed for evaluating our ability to perform three-dimensional computations of gravitational waves in spacetimes in which a black hole event horizon is present.
Additional Information
© 1998 American Physical Society. (Received 21 August 1997; published 18 December 1997) This work was supported by the NSF Binary Black Hole Grand Challenge Grant Nos. NSF PHY 93-18152/ASC 93-18152 (ARPA supplemented).Attached Files
Published - PhysRevD.57.1084.pdf
Submitted - 9712037.pdf
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Additional details
- Eprint ID
- 87499
- Resolver ID
- CaltechAUTHORS:20180629-155501427
- NSF
- PHY 93-18152
- NSF
- ASC 93-18152
- Advanced Research Projects Agency (ARPA)
- Created
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2018-06-29Created from EPrint's datestamp field
- Updated
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2021-11-15Created from EPrint's last_modified field