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  Calculating the gravitational self force in Schwarzschild spacetime

Barack, L., Mino, Y., Nakano, H., Ori, A., & Sasaki, M. (2002). Calculating the gravitational self force in Schwarzschild spacetime. Physical Review Letters, 88: 091101.

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Item Permalink: http://hdl.handle.net/11858/00-001M-0000-0013-5478-2 Version Permalink: http://hdl.handle.net/11858/00-001M-0000-0013-5479-F
Genre: Journal Article

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2769.pdf (Publisher version), 90KB
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 Creators:
Barack, Leor1, Author
Mino, Yasushi, Author
Nakano, Hiroyuki, Author
Ori, Amos, Author
Sasaki, Misao, Author
Affiliations:
1Astrophysical Relativity, AEI-Golm, MPI for Gravitational Physics, Max Planck Society, escidoc:24013              

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 Abstract: We present a practical method for calculating the local gravitational self-force (often called "radiation-reaction force") for a pointlike particle orbiting a Schwarzschild black hole. This is an implementation of the method of mode-sum regularization, in which one first calculates the (finite) contribution to the force due to each individual multipole mode of the perturbation, and then applies a certain regularization procedure to the mode sum. Here we give the values of all the "regularization parameters" required for implementing this regularization procedure, for any geodesic orbit in Schwarzschild spacetime

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Language(s): eng - English
 Dates: 2002
 Publication Status: Published in print
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 Identifiers: eDoc: 2769
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Title: Physical Review Letters
Source Genre: Journal
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Pages: - Volume / Issue: 88 Sequence Number: 091101 Start / End Page: - Identifier: -