arXiv (All)
open access
Properties of rapidly rotating hot neutron stars within Brueckner theory
We study the properties of hot rapidly rotating neutron stars using various equations of state based on the Brueckner-Hartree-Fock approach at finite temperature. The temperature dependence of gravitational mass, equatorial radius, Kepler frequency, moment of inertia are analysed in detail and unive
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
- 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
- Structural quasi-universality in highly magnetized differentially rotating neutron stars#1104464
- What We Have Learned from NICER About Neutron Star Radii#1131011
- Approximating neutron-star radii using gravitational-wave only measurements with symbolic regression#1084007
Record · ID 1156848
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