Newtonian hydrostatic equilibrium equation

E966302 UNEXPLORED

The Newtonian hydrostatic equilibrium equation is the classical relation in stellar structure that balances the inward pull of gravity with the outward pressure gradient in a spherically symmetric, non-relativistic fluid.

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Tolman–Oppenheimer–Volkoff equation → generalizationOf → Newtonian hydrostatic equilibrium equation ⓘ