Black holes in Gauss-Bonnet and Chern-Simons-scalar theory
Abstract
We carry out the stability analysis of the Schwarzschild black hole in Gauss-Bonnet and Chern-Simons-scalar theory. Here, we introduce two quadratic scalar couplings (φ12,φ22) to Gauss-Bonnet and Chern-Simons terms, where the former term is parity-even, while the latter one is parity-odd. The perturbation equation for the scalar φ1 is the Klein-Gordon equation with an effective mass, while the perturbation equation for φ2 is coupled to the parity-odd metric perturbation, providing a system of two coupled equations. It turns out that the Schwarzschild black hole is unstable against φ1 perturbation, leading to scalarized black holes, while the black hole is stable against φ2 and metric perturbations, implying no scalarized black holes.
Turn this paper into a lesson
ArcXiv compiles a structured reading guide from this paper's metadata: plain-English importance, contributions, prerequisite concepts, which sections to read first, flashcards, and a quiz. Grounded in the abstract, never invented.