Astrophysical assumptions and equation of state framework have larger impact on equation of state inference than individual neutron star observations
astro-ph.HE, gr-qc
Submitted: 2024-05-27
Updated: 2025-11-06
Comments: 24 pages, 19 figures
Code: https://github.com/oshaughn/research-projects-RIT
License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Terminology
Sources
- Hierarchical Triples as Early Sources of $r$-process Elements
- Inference of multi-channel r-process element enrichment in the Milky Way using binary neutron star merger observations
- The Accuracy of Neutron Star Radius Measurement with the Next Generation of Terrestrial Gravitational-Wave Observatories
- Modern tools for computing neutron star properties
- Rapid and accurate parameter inference for coalescing, precessing compact binaries
- A NICER view of the 1.4 solar-mass edge-on pulsar PSR J0614-3329
- Joint Electromagnetic and Gravitational Wave Inference of Binary Neutron Star Merger GW170817 Using Forward-Modeling Ejecta Predictions
- Inference on neutron star parameters and the nuclear equation of state with RIFT, using prior EOS information
- Narrowing RIFT: Focused simulation-based-inference for interpreting exceptional GW sources
- Inferring the neutron star equation of state simultaneously with the population of merging neutron stars
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