Application of Ryu-Takayanagi formula reveals a Page transition linked to black holes in RS1 geometry, suggesting new insights into surface dynamics.
We apply the Ryu-Takayanagi (RT) formula to CCEGA black stars in the Randall-Sundrum RS1 geometry. Two competing extremal surfaces are identified: a trivial surface on the IR brane and a non-trivial UV-anchored surface. Their crossing defines a Page transition at t_Page ~ 10^83 years for a 7 M_sun black star, with S_Page ~ 10^77 consistent with Bekenstein-Hawking. The rho_c surface acts spontaneously as a Penington island without being imposed — it emerges from the RS1 radion geometry. Exploratory result with all assumptions stated explicitly.
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Marc López Sánchez (2026) studied this question.
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