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- W4327744180 abstract "The superradiant instabilities of Kerr-Newman black holes with charged or uncharged massive spin-0 fields are calculated analytically to the next-to-leading order in the limit of $ensuremath{alpha}ensuremath{sim}{r}_{g}ensuremath{mu}ensuremath{ll}1$. A missing factor of $1/2$ in the previous leading-order result is identified. The next-to-leading order result has a compact form and is in good agreement with existing numerical calculations. The percentage error increases with $ensuremath{alpha}$, from a few percent for $ensuremath{alpha}ensuremath{sim}0.1$ to about 50% for $ensuremath{alpha}ensuremath{sim}0.4$. Massive neutral scalars too heavy to be produced with Kerr black hole superradiance may exist in the superradiant region of Kerr-Newman black holes." @default.
- W4327744180 created "2023-03-18" @default.
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- W4327744180 date "2023-03-17" @default.
- W4327744180 modified "2023-09-30" @default.
- W4327744180 title "Next-to-leading-order solution to Kerr-Newman black hole superradiance" @default.
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- W4327744180 doi "https://doi.org/10.1103/physrevd.107.064037" @default.
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