Cosmic Data Rendering: The Impact of Quantum Entanglement at the Black Hole Boundary on the Expansion of De Sitter Space

While modern holographic cosmology has been successfully demonstrated in Anti-de Sitter (AdS) space, it faces a fundamental challenge in the realistic De Sitter (dS) space—which possesses a positive cosmological constant and exhibits accelerated expansion—due to the inability to specify a global screen upon which information can be projected. This study proposes redefining the holographic screen of the expanding universe not at the unreachable boundary of cosmic infinity, but at the "local event horizons" of black holes distributed throughout the universe like a network. By integrating the ER=EPR hypothesis with the Complexity=Volume (CV) conjecture and holographic black hole lattice models, this paper elucidates a mechanism where the accelerated expansion of the universe is not a blind repulsive phenomenon caused by unknown dark energy. Rather, it is an information-theoretic and thermodynamic evolutionary process. As backend data (entanglement entropy) increases at local event horizons, the connected quantum wormholes (ER bridges) undergo volumetric expansion to accommodate the computational complexity, fundamentally compelling the macroscopic bulk space—the frontend universe—to expand its own rendering capacity.