Interior Entropy Evolution of a Cosmic-String-Pierced Loop Quantum Black Hole
How the interior entropy of a black hole, defined from its maximal enclosed spatial volume, evolves against the Bekenstein-Hawking horizon entropy during Hawking radiation, computed for a loop-quantum-corrected Schwarzschild metric threaded by a straight cosmic string. The learner sees how the cosmic string's conical deficit changes the relation between the two entropies and how the second law of thermodynamics is checked for their combined variation.
2501.00422
This paper studies the interior entropy of a black hole, a proposed handle on the information problem defined from the maximal interior spatial volume enclosed by the horizon rather than from the hor…