Probing black holes via quasinormal modes in a dark energy-induced dark matter
arXiv:2412.07172 · doi:10.1140/epjc/s10052-025-13953-0
Abstract
This study delves into the existence of dark matter around supermassive black holes in galactic cores using a novel gravitational model. By analyzing gravitational waves emitted during the ringdown phase of black holes under different field perturbations, we explore the potential for detecting dark matter. The model hypothesizes that the dark matter distribution around black hole is driven by a mechanism where dark energy endows gravitons with mass, thereby forming a new spacetime structure. Results reveal that as relevant parameters increase, the quasinormal modes (QNMs) exhibit a gradual reduction in real parts, with negative imaginary parts whose absolute values also decrease. Moreover, compared to gravitational wave signals from Schwarzschild black hole without dark matter, this system demonstrates significant differences in oscillation modes and frequencies. This achievement not only validates the self-consistency of the new gravitational model but also lays a theoretical foundation for subsequent gravitational wave detection within dark matter. Simultaneously, it provides new theoretical support for understanding the mechanism of dark energy in large-scale cosmic structures and broadens the research perspective on the relationships between black hole physics, dark matter, and dark energy.
References in corpus (18)
- Science Case for the Einstein Telescope
- Shadow of a black hole surrounded by dark matter
- Dynamics of test particles around a Bardeen black hole surrounded by perfect fluid dark matter
- Modelling the Sgr A* Black Hole Immersed in a Dark Matter Spike
- Dark matter spikes in the vicinity of Kerr black holes
- Probing hairy black holes caused by gravitational decoupling using quasinormal modes and greybody bounds
- Inflationary Butterfly Effect: Non-perturbative Dynamics From Small-Scale Features
- Gravitational ringing and superradiant instabilities of the Kerr-like black holes in a dark matter halo
- Observational constraints on Yukawa cosmology and connection with black hole shadows
- Scalar Perturbations of a Single-Horizon Regular Black Hole
- Apparent and emergent dark matter around a Schwarzschild black hole
- Ringdown of Charged Compact Objects using Membrane Paradigm
- Probing black holes in a dark matter spike of M87 using quasinormal modes
- Dark Universe Phenomenology from Yukawa Potential?
- Modeling the black holes surrounded by a dark matter halo in the galactic center of M87
- Probing the black holes in a dark matter halo of M87 using gravitational wave echoes
- Addressing the Hubble tension in Yukawa cosmology?
- Graviton mass due to dark energy as a superconducting medium: theoretical and phenomenological aspects