Abstract
Supermassive black holes can be seen as an agent of galaxy transformation. In particular, a supermassive black hole can cause a triaxial galaxy to evolve toward axisymmetry by inducing chaos in centrophilic orbit families. This is one way in which a single supermassive black hole can induce large-scale changes in the structure of its host galaxy-changes on scales far larger than the Schwarzschild radius (O(10−5)pc) and the radius of influence of the black hole (O(1)–O(100)pc).
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