arXiv (All)
open access
Neutron Economy and Freeze-out Dynamics in the Late-Time Cold r-Process
Standard r-process models often treat the freeze-out phase as a passive, uniform smoothing of the global abundance pattern. We demonstrate, however, that the final pattern is instead actively sculpted by a dynamic ``neutron economy'' that operates well after the free neutron source is exhausted. By
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
- Medium effects on neutron star modified and direct Urca cooling rates#1119411
- Outer-crust equations of state for neutron stars#1143741
- Correlated and uncorrelated Monte Carlo neutron capture rate variations in weak $\textit{r}$-process simulations#1050818
- A Data-Driven Model for $r$-Process Production Patterns#927467
- Warm Absorbers in Active Galactic Nuclei#639336
Record · ID 1106164
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