arXiv (All)
open access
Black hole thermodynamics at null infinity. Part 2: Open systems, Markovian dynamics and work extraction from non-rotating black holes
Black hole thermodynamics provides a unique setting in which general relativity, quantum field theory, and statistical mechanics converge. In semiclassical gravity, this interplay culminates in the generalized second law (GSL), whose modern proofs rely on information theoretic techniques applied to
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
- Black hole thermodynamics at null infinity. Part 1: Dual Generalized Second Law#999188
- Thermodynamic geometry as the missing link: toward a unified framework for black hole first-order phase transitions#1105702
- Kinetic Quantum Displacement (KQD): A New Framework for Chronogenesis and Gravitational Equilibrium in Black Holes#722247
- Large-$N$ Carrollian Thermodynamics from AdS Black-Hole Phase-Space Contractions#1084267
- Thermodynamics of Hairy Black Holes in Quantum Regimes: Insights from Horndeski Theory#987621
Record · ID 999189
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