Quasibound states of scalar fields in the consistent 4D Einstein-Gauss-Bonnet-(Anti-)de Sitter gravity
arXiv:2205.15613 · doi:10.1140/epjc/s10052-022-10650-0
Abstract
We examine the interaction between massless scalar fields and the gravitational field generated by a black hole solution that was recently obtained in the consistent well-defined 4-dimensional Einstein-Gauss-Bonnet gravity with a cosmological constant. In order to do this, we calculate quasibound state frequencies of scalar fields for the spherically symmetric black hole in the consistent 4-dimensional Einstein-Gauss-Bonnet-de Sitter and Anti-de Sitter theories. The expression for the quasibound states is obtained by using the polynomial condition associated to the Heun functions, and their values are overdamped. We also demonstrate the stability of the systems.
30 pages, 14 figures. arXiv admin note: text overlap with arXiv:2112.08711
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Cited by in corpus (5)
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- Quasibound States, Stability and Wave Functions of the Test Fields in the Consistent 4D Einstein-Gauss-Bonnet Gravity
- Perturbing the vortex: quasinormal and quasibound spectra of rotating acoustic geometries
- Quasibound states of analytic black-hole configurations in three and four dimensions