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In the present work we apply non extensive statistics to obtain equations ofstate suitable to describe stellar matter and verify its effects on microscopicand macroscopic quantities. Two snapshots of the star evolution are consideredand the direct Urca process is investigated with two different parameter sets.$q$-values are chosen as 1.05 and 1.14. The equations of state are onlyslightly modified, but the effects are enough to produce stars with slightlyhigher maximum masses. The onsets of the constituents are more stronglyaffected and the internal stellar temperature decreases with the increase ofthe $q$-value, with consequences on the strangeness and cooling rates of thestars.

Non extensive thermodynamics and neutron star properties