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Covariant phase space analysis of static spherical vacua in power-law $f(R)$ gravity
We formulate the static, spherically symmetric vacuum equations of power-law metric $f(R)$ gravity as a covariant autonomous system using the $(1+1+2)$ formalism. The finite critical sets include the scale-invariant Clifton--Barrow solution, a Minkowski endpoint shared by the Schwarzschild family, a
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