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In this work we construct an ultracompact star configuration in the frameworkof Gravitational Decoupling by the Minimal Geometric Deformation approach. Weuse the complexity factor as a complementary condition to close the system ofdifferential equations. It is shown that for a polynomial complexity theresulting solution can be matched with two different modified-vacuumgeometries.

Ultracompact stars with polynomial complexity by gravitational decoupling