AdS graviton stars and differential configurational entropy

Abstract

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.

6 pages, 1 figure

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Cited by in corpus (8)

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• Configurational entropy and the $N^{\ast }(1440)$ Roper resonance in QCD
• Quark stars in $D_3$-$D_7$ holographic model
• Configurational entropy and stability conditions of fermion and boson stars
• Statistical complexity as a probe of mass and phase structure in compact objects