arXiv (OAI Expanded)
open access
Approximating neutron-star radii using gravitational-wave only measurements with symbolic regression
Gravitational waves emitted by binary neutron-star inspirals carry information on components' masses and tidal deformabilities, but not directly radii, which are measured by electromagnetic observations of neutron stars. To improve the multi-messenger astronomy studies of neutron stars, an expressio
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
- Constraining the Equation of State of Neutron Stars with third-generation Gravitational Wave detectors#973950
- How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition#1130609
- 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
- Too small to fail: characterizing sub-solar mass black hole mergers with gravitational waves#986761
Record · ID 1084007
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