arXiv (All)
open access
Ruling out nucleonic direct Urca cooling in low-mass neutron stars using nuclear data
Connecting nuclear experiments to neutron star composition requires controlling the extrapolation of experimental information beyond the densities probed in the laboratory. We combine a broad set of nuclear structure observables and INDRA-FAZIA isospin-transport data within a Bayesian inference of t
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
- Neutron polarisation correction to triple-axis data with analytical derivations#176802
- Neutron radiographs of B12W and M8N socket sections of the Arecibo telescope#1054707
- Lightcurve Modelling of 2,205 ZTF DR2 Type~Ia Supernovae: Implications for SN Ia Physics and Cosmology#1070757
- The Impact of Errors in the Shape Function of Rotating Neutron Stars in the Oblate Schwarzschild Approximation#781039
- The Impact of Errors in the Shape Function of Rotating Neutron Stars in the Oblate Schwarzschild Approximation#779664
Record · ID 1051335
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