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The structure of a star composed of locally non-electroneutral incompressiblethree-component matter is considered within the framework of generalrelativity. For thermodynamic quantities like the pressure, the solution can berepresented as a series in the small parameter $1/\Lambda_{\mathrm G}\sim10^{-36}$, where the first approximation is the well-known electroneutralsolution. However, the equilibrium equations for the chemical potentials of thematter components, as it turns out, contain finite contributions fromnon-electroneutrality effects even in the zeroth order. Analytical solutionshave been obtained for all of the parameters of the problem underconsideration, which are illustrated by numerical examples.

Structure of Relativistic Stars Composed of Incompressible Matter in the Absence of Strict Electroneutrality