Quasinormal modes of black holes in Horndeski gravity
We study the perturbations to General Relativistic black holes (i.e. those without scalar hair) in Horndeski scalar-tensor gravity. First, we derive the equations of odd and even parity perturbations of both the metric and scalar field in the case of a Schwarzschild black hole, and show that the gra...
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| Format: | Journal article |
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American Physical Society
2018
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