A Newtonian reduction using angle-averaged centrifugal support as an effective anisotropy term enables 1D computation of rotating white dwarf sequences with the Chandrasekhar EOS, yielding percent-level mass and radius increases at high central densities.
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Rotation-Induced Effective Anisotropy in White Dwarfs as a Newtonian Benchmark with Relativistic Scale Assessment
A Newtonian reduction using angle-averaged centrifugal support as an effective anisotropy term enables 1D computation of rotating white dwarf sequences with the Chandrasekhar EOS, yielding percent-level mass and radius increases at high central densities.