arXiv (All)
open access
Entanglement and apparent thermality in simulated black holes
general-relativity-and-quantum-cosmologyhigh-energy-physics-theoryquantum-physicsstrongly-correlated-electrons
We investigate the apparent thermality of Hawking radiation in the semi-classical limit of quantum black holes using the mean-field limit of a chiral spin-chain simulator, which models fermions propagating on a black hole space-time in the continuum. In this free-theory regime, no genuine thermalisa
Conceptio Open Archive
Analyze & explore related research in Conceptio
Connect this record directly into your research workflow or AI agent. Explore citations across open repositories, query full text, and export structured proof bundles.
This document is indexed with metadata only: full text is not available in the archive for this record. Open the official source ↗
Related documents
- No model-independent evidence for a peak in binary black hole spin (mis)alignments#629996
- Entanglement in the $θ$-vacuum#1343542
- Deep thermalization and Hilbert space ergodicity#1078319
- Exploring Planckian Thermalization Time in Strongly Coupled Open Quantum Systems#433040
- Testing Van der Waals black holes using black hole photon rings#1051590
Record · ID 1357041
Retrieved via Conceptio: every document is proof-bundled with source, license, and retrieval metadata.
Retrieved via Conceptio: every document is proof-bundled with source, license, and retrieval metadata.
Bring this data into your agent: Connect via MCP or API · 20 free credits to start · no card required
Read the Docs → · View CLI source on GitHub · Conceptio Open Knowledge Archive
Read the Docs → · View CLI source on GitHub · Conceptio Open Knowledge Archive