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Stationary Scalar Clouds Around Rotating Black Holes

5 Pith papers cite this work. Polarity classification is still indexing.

5 Pith papers citing it
abstract

Motivated by novel results in the theory of wave dynamics in black-hole spacetimes, we analyze the dynamics of a massive scalar field surrounding a rapidly rotating Kerr black hole. In particular, we report on the existence of stationary (infinitely long-lived) regular field configurations in the background of maximally rotating black holes. The effective height of these scalar "clouds" above the central black hole is determined analytically. Our results support the possible existence of stationary scalar field dark matter distributions surrounding rapidly rotating black holes.

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gr-qc 5

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UNVERDICTED 5

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representative citing papers

Gravitational Atoms from Topological Stars

gr-qc · 2025-11-13 · unverdicted · novelty 5.0

Bound states of a massive scalar field around topological stars form strictly normal modes, producing a hydrogen-like spectrum when the Compton wavelength exceeds the star size and localized states otherwise.

Superradiance -- the 2020 Edition

gr-qc · 2015-01-26 · unverdicted · novelty 4.0

Black-hole superradiance extracts energy via the ergoregion and can trigger instabilities with applications to dark matter, beyond-Standard-Model physics, and laboratory analogs.

Dynamical Boson Stars

gr-qc · 2012-02-27 · unverdicted · novelty 2.0

Boson stars are particle-like solutions in general relativity that model dark matter, black hole mimickers, and binary systems.

Black hole spectroscopy: from theory to experiment

gr-qc · 2025-05-29 · unverdicted · novelty 2.0

A review summarizing the state of the art in black hole quasinormal modes, ringdown waveform modeling, current LIGO-Virgo-KAGRA observations, and prospects for LISA and next-generation detectors.

citing papers explorer

Showing 5 of 5 citing papers.

  • Splitting the Gravitational Atom: Instabilities of Black Holes with Synchronized or Resonant Hair gr-qc · 2025-09-24 · unverdicted · none · ref 27 · internal anchor

    Black holes with synchronized or resonant scalar hair exhibit dynamical splitting in which the horizon is ejected from the bosonic cloud center in the very hairy regime.

  • Gravitational Atoms from Topological Stars gr-qc · 2025-11-13 · unverdicted · none · ref 88 · internal anchor

    Bound states of a massive scalar field around topological stars form strictly normal modes, producing a hydrogen-like spectrum when the Compton wavelength exceeds the star size and localized states otherwise.

  • Superradiance -- the 2020 Edition gr-qc · 2015-01-26 · unverdicted · none · ref 109 · internal anchor

    Black-hole superradiance extracts energy via the ergoregion and can trigger instabilities with applications to dark matter, beyond-Standard-Model physics, and laboratory analogs.

  • Dynamical Boson Stars gr-qc · 2012-02-27 · unverdicted · none · ref 267 · internal anchor

    Boson stars are particle-like solutions in general relativity that model dark matter, black hole mimickers, and binary systems.

  • Black hole spectroscopy: from theory to experiment gr-qc · 2025-05-29 · unverdicted · none · ref 169

    A review summarizing the state of the art in black hole quasinormal modes, ringdown waveform modeling, current LIGO-Virgo-KAGRA observations, and prospects for LISA and next-generation detectors.