Published March 27, 2013
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Time domain calculation of the electromagnetic self-force on eccentric geodesics in Schwarzschild spacetime
- Creators
-
Haas, Roland
Abstract
I calculate the self-force acting on a particle with electric charge q moving on a generic geodesic around a Schwarzschild black hole. Using methods similar to those developed for the scalar field case discussed in a previous paper, I investigate the relative sizes of the conservative (half-advanced plus half-retarded) and dissipative (half-advanced minus half-retarded) pieces of the self-force. I also display the regularization parameters used in the mode-sum regularization scheme.
Additional Information
Imported from arXiv I thank Eric Poisson and Steve Detweiler for useful discussions and suggestions. I gratefully acknowledge support by the Natural Sciences and Engineering Council of Canada. This work was supported in part by NSF grants PHY-0903973 and PHY-0904015. This work was made possible by the facilities of the Shared Hierarchical Academic Research Computing Network (SHARCNET: www.sharcnet.ca) as well as the e FoRCE cluster at Georgia Tech.Attached Files
Submitted - 1112.3707.pdf
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Additional details
- Eprint ID
- 37384
- Resolver ID
- CaltechAUTHORS:20130307-144342936
- Natural Sciences and Engineering Council of Canada
- PHY-0903973
- NSF
- PHY-0904015
- NSF
- Created
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2013-03-27Created from EPrint's datestamp field
- Updated
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2023-06-02Created from EPrint's last_modified field
- Caltech groups
- TAPIR