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 () 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 is the Klein-Gordon equation with an effective mass, while the perturbation equation for 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 perturbation, leading to scalarized black holes, while the black hole is stable against and metric perturbations, implying no scalarized black holes.

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