  AdS graviton stars are studied in the differential configurational entropy
setup, as solutions of the effective Einstein field equations that backreact to
compactification. With the critical central density of AdS graviton stars, the
differential configurational entropy is derived and computed, presenting global
minima for a wide range of stellar mass magnitude orders. It indicates insular
domains of configurational stability for AdS graviton stars near astrophysical
neutron star densities. Other relevant features are also reported.
