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- W3039779904 abstract "Within general relativity, the unique stationary solution of an isolated black hole is the Kerr spacetime, which has a peculiar multipolar structure depending only on its mass and spin. We develop a general method to extract the multipole moments of arbitrary stationary spacetimes and apply it to a large family of horizonless microstate geometries. The latter can break the axial and equatorial symmetry of the Kerr metric and have a much richer multipolar structure, which provides a portal to constrain fuzzball models phenomenologically. We find numerical evidence that all multipole moments are typically larger (in absolute value) than those of a Kerr black hole with the same mass and spin. Current measurements of the quadrupole moment of black-hole candidates could place only mild constraints on fuzzballs, while future gravitational-wave detections of extreme mass-ratio inspirals with the space mission LISA will improve these bounds by orders of magnitude." @default.
- W3039779904 created "2020-07-10" @default.
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- W3039779904 date "2020-11-24" @default.
- W3039779904 modified "2023-10-02" @default.
- W3039779904 title "Distinguishing Fuzzballs from Black Holes through Their Multipolar Structure" @default.
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- W3039779904 doi "https://doi.org/10.1103/physrevlett.125.221601" @default.
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