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Cited by 356

The DOI matches its Crossref record; 29 of the 29 references it cites were found in a registry or an index.

Vector potential and metric perturbations of a rotating black hole

Chrzanowski, Paul L.·1975·Physical Review D
DOI 10.1103/physrevd.11.2042
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Abstract

The assumption of factorized Green's functions together with the inhomogeneous Teukolsky equations are used to derive analytic expressions for homogeneous metric (and vector potential) perturbations of a Kerr black hole. These homogeneous solutions are used to construct solutions to the perturbation equations when sources are present. What one finds are particularly simple formulas for the energy and angular momentum flux in the asymptotic regions ${r}^{*}\ensuremath{\rightarrow}\ifmmode\pm\else\textpm\fi{} \ensuremath{\infty}$.

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Metadata

Authors
Chrzanowski, P. L.
Venue
Physical Review D
Publisher
American Physical Society (APS)
Published
1975-04-15
Volume
11
Issue
8
Pages
2042-2062
ISSN
0556-2821 (ISSN-L)
DOI
10.1103/physrevd.11.2042
OpenAlex
W2045244268
Cited by
356
References
29
FWCI
8.21
Type
journal article
Language
en
Open access
closed

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CoChat. (2026). Citation check: Vector potential and metric perturbations of a rotating black hole. https://app.cochat.ai/papers/10.1103/physrevd.11.2042
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Chrzanowski, P. L. (1975). Vector potential and metric perturbations of a rotating black hole. Physical Review D. https://doi.org/10.1103/physrevd.11.2042

Data sources

Bibliographic data: Semantic Scholar, OpenAlex, Crossref.

Contains information from the Semantic Scholar Academic Graph Datasets, made available under the ODC Attribution License (ODC-BY 1.0).

Semantic Scholar’s data is described in: Kinney, R., et al. (2023). The Semantic Scholar Open Data Platform. arXiv:2301.10140.