Gravitational hair from extended geometric deformation lowers the Hawking temperature and the Landauer one-bit erasure cost, raises the Bekenstein-Hawking entropy, and adds a small positive Reeb-Wolf finite-size correction.
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Reeb-Wolf Improved Landauer Principle for Hairy Black Holes via Gravitational Decoupling
Gravitational hair from extended geometric deformation lowers the Hawking temperature and the Landauer one-bit erasure cost, raises the Bekenstein-Hawking entropy, and adds a small positive Reeb-Wolf finite-size correction.