Localized scalar structures around static black holes
arXiv:2203.02803 · doi:10.1016/j.nuclphysb.2023.116090
Abstract
In this work we address a way to capture scalar field solutions on static spacetimes by using BPS formalism and relaxing the general covariance condition. We focus on configurations where the background geometry describes topological black holes and present both analytical and numerical solutions, in addition to discussing the use of conserved charges associated to such field configurations. The obtained solutions are radially stable and the zero-mode arising from the stability equation can be written analytically.
Matches published version in Nuclear Physics B
References in corpus (15)
- Spontaneously scalarised Kerr black holes
- Spontaneous scalarization of charged black holes at the approach to extremality
- Thermodynamical properties of hairy black holes in n spacetimes dimensions
- Higher dimensional black hole scalarization
- Radially symmetric scalar solitons
- Stability of Topological Black Holes
- Topological black hole in the theory with nonminimal derivative coupling with power-law Maxwell field and its thermodynamics
- Configurational entropy of skyrmions and half-skyrmions in planar magnetic elements
- Evading Derrick's theorem in curved space: Static metastable spherical domain wall
- BPS equations and solutions for Maxwell-scalar theory
- BPS solitons with internal structure in the gauged sigma model
- Maxwell-scalar device based on the electric dipole
- First-order solitons with internal structures in an extended Maxwell- model
- Novel way to construct spatially localized finite energy structures
- Modeling Dark Matter Halos with Nonlinear Field Theories
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- Effective Lifshitz black holes, hydrodynamics, and transport coefficients in fluid/gravity correspondence