Entanglement entropy in holographic moving mirror and Page curve
Ibrahim Akal, Yuya Kusuki, Noburo Shiba, Tadashi Takayanagi, Zixia Wei
TL;DR
The paper constructs a gravity dual for a 2D CFT with a moving mirror, modeling Hawking-like radiation and black-hole evaporation, and computes the time evolution of entanglement entropy. Using conformal maps, holographic AdS/BCFT with an end-of-the-world brane Q, and replica techniques, it demonstrates a Page-curve-like entropy evolution: linear growth from entangled-pair production and subsequent saturation due to island contributions, with explicit expressions in both free Dirac fermion and holographic CFTs. The brane-world interpretation links boundary entropy to an effective 2D gravitational sector and recasts the entropy evolution in terms of the island formula, offering a concrete strong-coupling realization of unitary black-hole radiation. The framework thus provides a tractable, holographic model to study unitarity and entropy dynamics in black hole evaporation, with avenues to incorporate singularities and gravitational radiation by adjusting the brane geometry.
Abstract
We calculate the time evolution of entanglement entropy in two dimensional conformal field theory with a moving mirror. For a setup modeling Hawking radiation, we obtain a linear growth of entanglement entropy and show that this can be interpreted as the production of entangled pairs. For a setup, which mimics black hole formation and evaporation, we find that the evolution follows the ideal Page curve. We perform these computations by constructing the gravity dual of the moving mirror model via holography. We also argue that our holographic setup provides a concrete model to derive the Page curve for black hole radiation in the strong coupling regime of gravity.
