A reduced 1D Newtonian model encodes centrifugal support in white dwarfs as pressure anisotropy Δ_rot = (1/3)ρ Ω² r², producing monotonic increases in limiting mass and radius with percent-level gains at f=0.35 while remaining sub-Keplerian.
Friedman, James R
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Rotation-Induced Pressure Anisotropy in Newtonian White Dwarfs: Sequences and Applicability Criteria
A reduced 1D Newtonian model encodes centrifugal support in white dwarfs as pressure anisotropy Δ_rot = (1/3)ρ Ω² r², producing monotonic increases in limiting mass and radius with percent-level gains at f=0.35 while remaining sub-Keplerian.