Probing the existence of ultralight bosons with a single gravitational-wave measurement
arXiv:1804.09659 · doi:10.1038/s41550-019-0712-4
Abstract
Light bosons, proposed as a possible solution to various problems in fundamental physics and cosmology, include a broad class of candidates for beyond the Standard Model physics, such as dilatons and moduli, wave dark matter and axion-like particles. If light bosons exist in nature, they will spontaneously form "clouds" by extracting rotational energy from rotating massive black holes through superradiance, a classical wave amplification process that has been studied for decades. The superradiant growth of the cloud sets the geometry of the final black hole, and the black hole geometry determines the shape of the cloud. Hence, both the black hole geometry and the cloud encode information about the light boson. For this reason, measurements of the gravitational field of the black hole/cloud system (as encoded in gravitational waves) are over-determined. We show that a single gravitational wave measurement can be used to verify the existence of light bosons by model selection, rule out alternative explanations for the signal, and measure the boson mass. Such measurements can be done generically for bosons in the mass range eV using LISA observations of extreme mass-ratio inspirals.
References in corpus (10)
- Cosmic Structure as the Quantum Interference of a Coherent Dark Wave
- Discovering the QCD Axion with Black Holes and Gravitational Waves
- Instability of the massive Klein-Gordon field on the Kerr spacetime
- Searching for dilaton dark matter with atomic clocks
- Probing Ultralight Bosons with Binary Black Holes
- Black holes as particle detectors: evolution of superradiant instabilities
- Constraining the mass of dark photons and axion-like particles through black-hole superradiance
- Gravitational waves as a probe of dark matter mini-spikes
- Orbital fingerprints of ultralight scalar fields around black holes
- Testing general relativity with gravitational waves: a reality check
Cited by in corpus (94)
- Testing the nature of dark compact objects: a status report
- Ultra-Light Dark Matter
- Wave Dark Matter
- New Horizons for Fundamental Physics with LISA
- The Spectra of Gravitational Atoms
- Rapid generation of fully relativistic extreme-mass-ratio-inspiral waveform templates for LISA data analysis
- Detecting fundamental fields with LISA observations of gravitational waves from extreme mass-ratio inspirals
- The Missing Link in Gravitational-Wave Astronomy: Discoveries waiting in the decihertz range
- Parametrized black hole quasinormal ringdown. II. Coupled equations and quadratic corrections for nonrotating black holes
- Disks, spikes, and clouds: distinguishing environmental effects on BBH gravitational waveforms
- Black Hole Spin Constraints on the Mass Spectrum and Number of Axion-like Fields
- The response of ultralight dark matter to supermassive black holes and binaries
- Directed searches for gravitational waves from ultralight bosons
- Black hole superradiant instability from ultralight spin-2 fields
- Gravitational wave probes of dark matter: challenges and opportunities
- The Science of the Einstein Telescope
- Wet Extreme Mass Ratio Inspirals May Be More Common For Spaceborne Gravitational Wave Detection
- Constraints on ultralight scalar bosons within black hole spin measurements from LIGO-Virgo's GWTC-2
- Dynamic Signatures of Black Hole Binaries with Superradiant Clouds
- Extreme Dark Matter Tests with Extreme Mass Ratio Inspirals
- Extreme mass-ratio inspirals into black holes surrounded by scalar clouds
- Dynamical Friction in Gravitational Atoms
- Scalar field effects on the orbit of S2 star
- Tidal deformability of dressed black holes and tests of ultralight bosons in extended mass ranges
- Detecting massive scalar fields with Extreme Mass-Ratio Inspirals
- Searching for ultralight bosons within spin measurements of a population of binary black hole mergers
- Impact of multiple modes on the black-hole superradiant instability
- A Unique Multi-Messenger Signal of QCD Axion Dark Matter
- SuperRad: Modeling the black hole superradiance gravitational waveform
- Probing the Nature of Black Holes: Deep in the mHz Gravitational-Wave Sky
- Black hole merger simulations in wave dark matter environments
- Probing Dark Matter Spikes via Gravitational Waves of Extreme Mass Ratio Inspirals
- Follow-up signals from superradiant instabilities of black hole merger remnants
- The effect of wave dark matter on equal mass black hole mergers
- Relativistic drag forces on black holes from scalar dark matter clouds of all sizes
- Directed search for continuous gravitational-wave signals from the Galactic Center in the Advanced LIGO second observing run
- Short Review of the main achievements of the Scalar Field, Fuzzy, Ultralight, Wave, BEC Dark Matter model
- Photon Ring Astrometry for Superradiant Clouds
- Relativistic perturbation theory for black-hole boson clouds
- Black hole superradiant instability for massive spin-2 fields
- Constraining properties of asymmetric dark matter candidates from gravitational-wave observations
- Quasibound states of charged dilatonic black holes
- Superradiance of charged black holes embedded in dark matter halos
- Can the GW190814 secondary component be a bosonic dark matter admixed compact star?
- Effective field theory for black holes with induced scalar charges
- Extreme mass ratio inspirals in galaxies with dark matter halos
- Improved Analytic Solution of Black Hole Superradiance
- Methods and prospects for gravitational wave searches targeting ultralight vector boson clouds around known black holes
- Searching for ultralight bosons with supermassive black hole ringdown
- Signatures of Ultralight Bosons in Compact Binary Inspiral and Outspiral
- Evolution of black hole shadows from superradiance
- Relativistic Mean Motion Resonance
- Evolution of diffuse scalar clouds around binary black holes
- Superradiant pion clouds around primordial black holes
- GW170817 and GW190425 as Hybrid Stars of Dark and Nuclear Matters
- A bright electromagnetic counterpart to extreme mass ratio inspirals
- The gravitational capture of compact objects by massive black holes
- Spinning Black Holes with Axion Hair
- Observational prospects of self-interacting scalar superradiance with next-generation gravitational-wave detectors
- Superradiant energy extraction from rotating hairy Horndeski black holes
- Detecting Fundamental Vector Fields with LISA
- Probing Ultralight Bosons with Compact Eccentric Binaries
- Probing fundamental physics with Extreme Mass Ratio Inspirals: a full Bayesian inference for scalar charge
- Testing gravity with Extreme-Mass-Ratio Inspirals
- Implication of nano-Hertz stochastic gravitational wave background on ultralight axion particles
- Stringent constraints on the light boson model with supermassive black hole spin measurements
- Quantum gravity phenomenology at the dawn of the multi-messenger era -- A review
- Getting More Out of Black Hole Superradiance: a Statistically Rigorous Approach to Ultralight Boson Constraints from Black Hole Spin Measurements
- Search for continuous gravitational wave signals from luminous dark photon superradiance clouds with LVK O3 observations
- Probing vector gravitational atoms with eccentric intermediate mass-ratio inspirals
- Piercing of a solitonic boson star by a black hole
- Resonant excitation of eccentricity in spherical extreme-mass-ratio inspirals
- On the origin of quasinormal modes in semi-open systems
- Methodology for constraining ultralight vector bosons with gravitational wave searches targeting merger remnant black holes
- Astrophysics with the Laser Interferometer Space Antenna
- Effects of Superradiance in Active Galactic Nuclei
- Self-interaction effects on the Kerr black hole superradiance and their observational implications
- Analytical model of precessing binaries using post-Newtonian theory in the extreme mass-ratio limit I: General Formalism
- Extreme mass ratio inspirals around topological stars
- Gravitational waves from superradiant instabilities of rotating black holes
- Field excitation in fuzzy dark matter near a strong gravitational wave source
- Science Potential for Stellar-mass Black Holes as Neighbors of Sgr A*
- Parametric-resonance based phenomenology of gravitating axion configurations
- Distinguishing dark matter halos with Extreme mass ratio inspirals
- Augmented analytic kludge waveform with quadrupole moment correction
- Dynamical friction from scalar dark matter in the relativistic regime
- Challenging theories of gravitation: dark matter, compact objects and gravitational waves
- The Effect of Mission Duration on LISA Science Objectives
- Preliminary forecasting constraint on scalar charge with LISA in non-vacuum environments
- Crossing the dark matter soliton core: a possible reversed orbital precession
- Extreme Mass Ratio Inspirals triggered by Massive Black Hole Binaries: from Relativistic Dynamics to Cosmological Rates
- Superradiant scattering of massive scalar field due to magnetically charged rotating black hole
- Extreme mass-ratio inspirals as probes of scalar fields: eccentric equatorial orbits around Kerr black holes
- Piercing of a boson star by a black hole