Nonminimal global monopole
arXiv:2307.13939 · doi:10.1103/PhysRevD.108.084002
Abstract
In this paper, we investigate the gravitational effects of a global monopole that couples nonminimally to gravity. Considering a coupling parameter of arbitrary strength, we have obtained an analytical solution for the field equations of the model in the asymptotic region outside the monopole's core, thus generalizing previous results. Within the weak coupling regime, we have also analyzed how this matter-geometry interplay affects some physical properties of the monopole, such as its radius and the mass enclosed in its core, which are explicitly computed and expressed in terms of the parameter of the theory. Using the Hahari-Loustó toy model, we have also found that the modification of general relativity (GR) may render a positive sign to the monopole mass, which means a global monopole able to exert attractive gravitational force on matter particles surrounding it. Next, we have studied some properties of a hairy black hole carrying such a global monopole charge. In this vein, we verified that the deviation from GR may provide such a spacetime with both event and Cauchy horizons, thus emulating a Reissner-Nordström framework. Finally, we have performed a study of the geodesic motion of timelike particles around this black hole by setting the conditions for stable circular orbits. We also examined the gravitational bending experienced by photons traveling through this geometry, taking into account finite-distance corrections on the deflection angle. Additionally, we make an order-of-magnitude estimate for this extra contribution considering the light bending caused by Sagittarius A*.
V4: 22 Pages, 6 figures; Text improved, typos corrected, results unchanged. Matches the published version
References in corpus (17)
- First M87 Event Horizon Telescope Results. I. The Shadow of the Supermassive Black Hole
- First M87 Event Horizon Telescope Results. VI. The Shadow and Mass of the Central Black Hole
- First M87 Event Horizon Telescope Results. IV. Imaging the Central Supermassive Black Hole
- First M87 Event Horizon Telescope Results. V. Physical Origin of the Asymmetric Ring
- First M87 Event Horizon Telescope Results. II. Array and Instrumentation
- Extra force in modified theories of gravity
- First M87 Event Horizon Telescope Results. III. Data Processing and Calibration
- Horndeski theory and beyond: a review
- Quasinormal modes and Strong Cosmic Censorship
- The Contribution of the Cosmological Constant to the Relativistic Bending of Light Revisited
- Finite-distance corrections to the gravitational bending angle of light in the strong deflection limit
- Thin accretion disks in f(R) modified gravity models
- Do f(R) theories matter?
- Accretion disks around black holes in modified strong gravity
- To conserve, or not to conserve: A review of nonconservative theories of gravity
- global monopole revisited
- Appearance of innermost stable circular orbits of accretion discs around rotating neutron stars
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