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.

中文翻译：

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AdS 引力子星和微分构型熵

AdS 引力子星在微分构型熵设置中被研究，作为对紧化有反向反应的有效爱因斯坦场方程的解。利用 AdS 引力子星的临界中心密度，推导出和计算微分构型熵，呈现大范围恒星质量数量级的全局最小值。它表明了 AdS 引力子星在天体物理中子星密度附近的构型稳定性的孤立域。还报告了其他相关功能。