Published May 21, 2008
| Submitted
Journal Article
Open
High accuracy simulations of Kerr tails: coordinate dependence and higher multipoles
Chicago
Abstract
We investigate the late-time behavior of a scalar field on a fixed Kerr background using a 2 + 1 dimensional pseudo-spectral evolution code. We compare evolutions of pure axisymmetric multipoles in both Kerr–Schild and Boyer–Lindquist coordinates. We find that the late-time power-law decay rate depends upon the slicing of the background, confirming previous theoretical predictions for those decay rates. The accuracy of the numerical evolutions is sufficient to decide unambiguously between competing claims in the literature.
Additional Information
© 2018 IOP Publishing. Received 19 December 2007, in final form 31 March 2008. Published 7 May 2008. This research was supported in part by NSF grant PHY 0505761 to Louisiana State University, by a grant from the Sherman Fairchild Foundation to Cornell, and by NSF grants PHY-0652952, DMS-0553677, PHY-0652929 and NASA grant NNG05GG51G at Cornell. The research employed the resources of the CCT at LSU, which is supported by funding from the Louisiana legislature's Information Technology Initiative. MT would like to thank Enrique Pazos and Jorge Pullin for helpful discussions throughout this project and hospitality at Cornell University, where this work was done.Attached Files
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Additional details
- Eprint ID
- 86849
- DOI
- 10.1088/0264-9381/25/10/105022
- Resolver ID
- CaltechAUTHORS:20180606-131328537
- NSF
- PHY-0505761
- Sherman Fairchild Foundation
- NSF
- PHY-0652952
- NSF
- DMS-0553677
- NSF
- PHY-0652929
- NASA
- NNG05GG51G
- Created
-
2018-06-06Created from EPrint's datestamp field
- Updated
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2022-07-12Created from EPrint's last_modified field