arXiv (OAI Expanded)
open access
Bayesian approach study of hybrid neutron stars
In this work, we explore how astronomical observations (specifically measurements of masses and radii) can constrain the presence of quark matter inside neutron stars, namely the phase transition from nuclear matter to deconfined quark matter. Our approach employs Bayesian analysis to study this con
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
- Bayesian Inferences on Analytical Equations of State Approximations of Neutron Stars#1149481
- Pulse profiles of accreting neutron stars - A review of analysis methods, observations, and theoretical models#662068
- Pulse profiles of accreting neutron stars - A review of analysis methods, observations, and theoretical models#661018
- NICER Constraints on Low density Interpolation and High density Continuation in Neutron Star Equations of State#1014736
- Trace Anomaly and Effective Topological Sources in Neutron Stars#659029
Record · ID 1108976
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