Probing vector hair of black holes with extreme mass ratio inspirals

Abstract

The bumblebee gravity model, with a vector field nonminimally coupled to gravity, is a natural extension of the Einstein-Maxwell theory. In this theory, a black hole can carry a vector hair, making the metric deviate from the Schwarzschild metric. To investigate the detectability of the vector hair, we consider an Extreme Mass Ratio Inspiral (EMRI) system, where a stellar-mass black hole inspiraling into a supermassive black hole. We find that, with a one-year observation of an EMRI by a space-based gravitational-wave detector, we can probe the vector charge as small as $Q\sim 10^{-3}$ in the bumblebee gravity model, which is about three orders of magnitude tighter comparing to current EHT observations.

8 pages, 4 figures

References in corpus (47)

• First M87 Event Horizon Telescope Results. I. The Shadow of the Supermassive Black Hole
• First Sagittarius A* Event Horizon Telescope Results. I. The Shadow of the Supermassive Black Hole in the Center of the Milky Way
• First M87 Event Horizon Telescope Results. VI. The Shadow and Mass of the Central Black Hole
• First M87 Event Horizon Telescope Results. V. Physical Origin of the Asymmetric Ring
• First M87 Event Horizon Telescope Results. VIII. Magnetic Field Structure near The Event Horizon
• First Sagittarius A* Event Horizon Telescope Results. VI: Testing the Black Hole Metric
• Can environmental effects spoil precision gravitational-wave astrophysics?
• Intermediate and Extreme Mass-Ratio Inspirals -- Astrophysics, Science Applications and Detection using LISA
• Signals for Lorentz Violation in Post-Newtonian Gravity
• Model Waveform Accuracy Standards for Gravitational Wave Data Analysis
• Constraints on black-hole charges with the 2017 EHT observations of M87*
• Gravitational Test Beyond the First Post-Newtonian Order with the Shadow of the M87 Black Hole
• Concepts and status of Chinese space gravitational wave detection projects
• New Horizons for Fundamental Physics with LISA
• Using LISA EMRI sources to test off-Kerr deviations in the geometry of massive black holes
• Black holes in galaxies: environmental impact on gravitational-wave generation and propagation
• Spontaneous Lorentz and Diffeomorphism Violation, Massive Modes, and Gravity
• Ultra Light Boson Dark Matter and Event Horizon Telescope Observations of M87*
• Gravitational waves from extreme-mass-ratio systems in astrophysical environments
• Detecting fundamental fields with LISA observations of gravitational waves from extreme mass-ratio inspirals
• Black holes in vector-tensor theories
• Detectable environmental effects in GW190521-like black-hole binaries with LISA
• Static spherical vacuum solutions in the bumblebee gravity model
• Gravitational-wave glitches in chaotic extreme-mass-ratio inspirals
• Gravitational waves from Extreme Mass Ratio Inspirals in non-pure Kerr spacetimes
• Extreme mass-ratio inspirals around a spinning horizonless compact object
• Gravitational wave cosmology with extreme mass-ratio inspirals
• Testing spacetime symmetry through gravitational waves from extreme-mass-ratio inspirals
• Polarizations of Gravitational Waves in the Bumblebee Gravity Model
• Science with the TianQin Observatory: Preliminary Results on Testing the No-hair Theorem with EMRI
• Multiband Observation of LIGO/Virgo Binary Black Hole Mergers in the Gravitational-wave Transient Catalog GWTC-1
• Static and rotating solutions for Vector-Galileon theories
• Probing Dark Matter Spikes via Gravitational Waves of Extreme Mass Ratio Inspirals
• Gravitational-wave glitches: resonant islands and frequency jumps in non-integrable extreme-mass-ratio inspirals
• Frequency response of space-based interferometric gravitational-wave detectors
• Analytic Kludge Waveforms for Extreme Mass Ratio Inspirals of Charged Object around Kerr-Newman Black Hole
• Prospects for determining the nature of the secondaries of extreme mass-ratio inspirals using the spin-induced quadrupole deformation
• Bumblebee field as a source of cosmological anisotropies
• Intermediate Mass-Ratio Inspirals with Dark Matter Minispikes
• Neutron stars in massive scalar-Gauss-Bonnet gravity: Spherical structure and time-independent perturbations
• Detection of scalar fields by Extreme Mass Ratio Inspirals with a Kerr black hole
• Comment on "Greybody radiation and quasinormal modes of Kerr-like black hole in Bumblebee gravity model"
• Extreme mass ratio inspirals into black holes surrounded by matter
• Detecting electric charge with Extreme Mass Ratio Inspirals
• Constraint on Brans-Dicke theory from intermediate/extreme mass ratio inspirals
• Chaos in Quadratic Gravity
• Reissner-Nordström perturbation framework with gravitational wave applications

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• Gravitational odd-parity perturbation of a Horndeski hairy black hole: quasinormal mode and parameter constraint
• Analytical model of precessing binaries using post-Newtonian theory in the extreme mass-ratio limit I: General Formalism
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• Generic effective sources for first-order in mass-ratio gravitational self-force calculations in Schwarzschild spacetime