Superradiant instability of area quantized Kerr black hole with discrete reflectivity
arXiv:2404.10742 · doi:10.1140/epjc/s10052-025-14204-y
Abstract
Ultralight bosons can condense to form the so-called bosonic clouds around spinning black holes by superradiance instability. When quantum effects are taken into account, the classical black holes were replaced by exotic compact objects including area quantized black holes. In this work, we consider the superradiant instabilities of massive scalar fields around area quantized Kerr black hole. We introduce the reflectivity of area quantized black hole possesses the distinct discrete feature, and the scalar fields have the superradiant modes solution only within the specific mass range. In addition, the area quantization may terminate the superradiance when the black hole spins down, or even suppress the formation of the bosionic cloud.
arXiv comment16 pages, 9 figures, published version in EPJC
References in corpus (56)
- Quasinormal modes of black holes and black branes
- String Axiverse
- Black Holes: Complementarity or Firewalls?
- Discreteness of area and volume in quantum gravity
- Quantum Geometry and Black Hole Entropy
- The Waning of the WIMP? A Review of Models, Searches, and Constraints
- Thermodynamical Aspects of Gravity: New insights
- TOPICAL REVIEW: General relativistic boson stars
- New experimental approaches in the search for axion-like particles
- Bohr's Correspondence Principle and The Area Spectrum of Quantum Black Holes
- Exploring the String Axiverse with Precision Black Hole Physics
- Black Hole Entropy from Loop Quantum Gravity
- Gravity and the Thermodynamics of Horizons
- Direct Detection of WIMP Dark Matter: Concepts and Status
- Spectroscopy of the quantum black hole
- The fuzzball proposal for black holes
- A review of indirect searches for particle dark matter
- Black holes as particle detectors: evolution of superradiant instabilities
- Gravitational Condensate Stars: An Alternative to Black Holes
- Black Hole Mergers and the QCD Axion at Advanced LIGO
- Perturbations of slowly rotating black holes: massive vector fields in the Kerr metric
- Stochastic and resolvable gravitational waves from ultralight bosons
- Dark Matter, Millicharges, Axion and Scalar Particles, Gauge Bosons, and Other New Physics with LDMX
- The Holographic Principle
- The Spectra of Gravitational Atoms
- Hawking emission of gravitons in higher dimensions: non-rotating black holes
- Gravitational Collider Physics
- Stimulated axion decay in superradiant clouds around primordial black holes
- Exotic Compact Objects and How to Quench their Ergoregion Instability
- Black hole state counting in Loop Quantum Gravity: A number theoretical approach
- Characterizing the continuous gravitational-wave signal from boson clouds around Galactic isolated black holes
- Ergoregion instability of exotic compact objects: electromagnetic and gravitational perturbations and the role of absorption
- Detailed black hole state counting in loop quantum gravity
- A first search for a stochastic gravitational-wave background from ultralight bosons
- Potential gravitational-wave signatures of quantum gravity
- Dynamic Signatures of Black Hole Binaries with Superradiant Clouds
- Modeling and searching for a stochastic gravitational-wave background from ultralight vector bosons
- The Black Hole Information Problem
- Flux-area operator and black hole entropy
- Effective Field Theory of Black Hole Echoes
- Relativistic perturbation theory for black-hole boson clouds
- Black hole superradiant instability for massive spin-2 fields
- Superradiant axion clouds around asteroid-mass primordial black holes
- Constraining Fundamental Physics with the Event Horizon Telescope
- Improved Analytic Solution of Black Hole Superradiance
- Spectral Lines of Quantized, Spinning Black Holes and their Astrophysical Relevance
- Imprint of black hole area quantization and Hawking radiation on inspiraling binary
- Signatures of Ultralight Bosons in Compact Binary Inspiral and Outspiral
- Gravitational atoms in the braneworld scenario
- Gravitational Waves and Possible Fast Radio Bursts from Axion Clumps
- Probing the quantum nature of black holes with ultra-light boson environments
- Near-horizon microstructure and superradiant instability of black holes
- Implication of nano-Hertz stochastic gravitational wave background on ultralight axion particles
- Superradiant instabilities of massive bosons around exotic compact objects
- Massive tensor field perturbations on extremal and near-extremal static black holes
- On the Interaction between Ultralight Bosons and Quantum-Corrected Black Holes