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Volumn 78, Issue 12, 2008, Pages

Two approaches for the gravitational self-force in black hole spacetime: Comparison of numerical results

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[No Author keywords available]

Indexed keywords

EID: 58949103287 PISSN: 15507998 EISSN: 15502368 Source Type: Journal
DOI: 10.1103/PhysRevD.78.124024 Document Type: Article

Times cited : (122)

References (17)

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14
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- Equation 2.7 only makes sense when ξα and ξ α are well defined on the worldline. It is not immediately clear how to define the GSF in gauges related to the Lorenz gauge through transformations ξα which do not satisfy these conditions. See Ref. for a discussion of this issue.
- Equation 2.7 only makes sense when ξα and ξ α are well defined on the worldline. It is not immediately clear how to define the GSF in gauges related to the Lorenz gauge through transformations ξα which do not satisfy these conditions. See Ref. for a discussion of this issue.

15
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16
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- The class ξ^α has been introduced before in the literature-see AppendixA of Ref..
- The class ξ^α has been introduced before in the literature-see AppendixA of Ref..

17
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- Barack, L.¹ Lousto, C.O.²

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