arXiv (All)
open access
Growth of a Black Hole on a Self-Gravitating Radiation
We feed a black hole on a self-gravitating radiation and observe what happens during the process. Considering a spherical shell of radiation, we show that the contribution of self-gravity makes the thermodynamic interaction through the bottom of the shell be distinguished from thermodynamic interact
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
- Thermal Quantum Fluctuations in Einstein-Nonlinear Maxwell-Yukawa Black Hole#987840
- Asymptotic description of a test particle around a Schwarzschild black hole#935725
- One-loop effect in the charged 2D black hole near extremality#986231
- Black Hole Horizon Étendue and the Geometric Limit of Radiometric Throughput#75078
- Monetary Policy Analysis in a Small Open Economy: A Dynamic Stochastic General Equilibrium Approach#499871
Record · ID 1062728
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