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• W1983482561 endingPage "2971" @default.
• W1983482561 startingPage "2963" @default.
• W1983482561 abstract "The electromagnetized Kerr metric is used to provide a model for the exterior spacetime of a rotating black hole immersed in an external electromagnetic field. As compared to the vacuum Kerr metric, the electromagnetic field neither changes the location nor the proper area of the event horizon. However, it pulls in the static limit. Further, for a suitable value of the electromagnetic field, no ergosphere can be formed. An algorithm is developed to analyze, using algebraic computing, the equatorial circular timelike and null geodesics. As an application, we study the test-particle motion around a supermassive rotating black hole immersed in a strong electromagnetic field. It is shown that the electromagnetic field enhances the test-particle release of energy, although it diminishes the probabilities of extraction of energy through the Penrose process." @default.
• W1983482561 created "2016-06-24" @default.
• W1983482561 creator A5003933357 @default.
• W1983482561 creator A5074764542 @default.
• W1983482561 date "1988-11-15" @default.
• W1983482561 modified "2023-09-25" @default.
• W1983482561 title "Rotating black hole in an external electromagnetic field" @default.
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• W1983482561 doi "https://doi.org/10.1103/physrevd.38.2963" @default.
• W1983482561 hasPubMedId "https://pubmed.ncbi.nlm.nih.gov/9959041" @default.
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