Instabilities of massive scalar perturbations of a rotating black hole
Integrity signals
Registry
Cites
Statistics
Claims the paper makes
Claims other papers make about this one
Each is checked against this paper’s own text: does it say what the citing paper says it does?
Black hole superradiance is a classical instability that draws energy from a spinning black hole and deposits it in field oscillations of a light scalar localized outside the horizon.
“Superradiance is a classical instability which draws energy from the black hole and deposits it in the field oscillations of a light scalar, localized in a spherical region outside the horizon.”
From Euclidean Wormholes, Baby Universes, and Their Impact on Particle Physics and Cosmology (2018) · cites this paper as Zouros and Eardley, 1979
For an extremal black hole and R ≫ 1/m, the instability time scale is τ ≃ (10^7 R) exp(1.84 mR).
“For an extremal black hole and R ≫ 1/m, the instability time scale is given by Zouros and Eardley (1979) τ ≃ (10 7 R) exp (1.84 mR).”
From Euclidean Wormholes, Baby Universes, and Their Impact on Particle Physics and Cosmology (2018) · cites this paper as Zouros and Eardley, 1979
The citation lists haven’t been fetched yet
References 18 · Cited by 355
- Authors
- Zouros, T. J. M., & Eardley, D. M.
- Affiliations
- Yale University (US)
- Venue
- Annals of Physics
- Publisher
- Elsevier BV
- Published
- 1979-03
- Volume
- 118
- Issue
- 1
- Pages
- 139-155
- ISSN
- 0003-4916 (ISSN-L)
- OpenAlex
- W1970192599
- Cited by
- 355
- References
- 18
- Citations by year
- 2026: 21 · 2025: 29 · 2024: 26 · 2023: 21 · 2022: 24 · 2021: 25 · 2020: 24 · 2019: 16 · 2018: 19 · 2017: 17 · 2016: 15 · 2015: 27 · 2014: 22 · 2013: 13 · 2012: 11
- FWCI
- 1.15
- Type
- journal article
- Language
- en
- Open access
- closed
- Locations
- Annals of Physics (publishedVersion)
- Topics
- Physical Sciences › Physics and Astronomy › Nuclear and High Energy Physics › Black Holes and Theoretical Physics
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Astrophysical Phenomena and Observations
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Pulsars and Gravitational Waves Research
- Keywords
- massive scalar field, rotating black holes, black hole stability, superradiance, wave packets, WKB approximation, particle creation, energy conservation (physics)
About these checks
Registry, retraction, Cites and statistics results are computed, not judged, with one exception: a printed reference that no index lists is read once by a model before it counts as a citation error. Claims are extracted by a model and kept only when their quote appears verbatim in the text; each cited source is then checked, with a model’s help, for whether it says what the claim relies on. Those verdicts can be wrong — read the claim’s quote and the cited source before relying on one.
Statistics and arithmetic are recomputed, not judged.
Confidence bands are shown only for fields calibrated on our annotated test set. None is calibrated yet, so no band is shown.
What counts as a claim ›How we measure confidence ›How we check this ›
Are you an author, or do you see a problem with this page? Request a review