Constraining equation of state of neutron star using neutron star-black hole mergers
gr-qc, astro-ph.HE
Submitted: 2026-08-31
Updated: 2026-08-31
License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Terminology
Sources
- TROYE: Modeling Dynamic Phase Transitions in Gravitational Waves from Neutron Star-Black Hole Mergers
- Nuclear physics with gravitational waves from neutron stars disrupted by black holes
- Investigating the detection rates and inference of gravitational-wave and radio emission from black hole neutron star mergers
- Detection of Gravitational Wave modes in third generation detectors
- Characterizing Gravitational Wave Detector Networks: From A$^\sharp$ to Cosmic Explorer
- Constraints on the Neutron Star Equation of State from GW170817
- Tidal response of regular black holes
- Optimizing Bayesian model selection for equation of state of cold neutron stars
- Bilby: A user-friendly Bayesian inference library for gravitational-wave astronomy
- Constraining the neutron star-black hole merger rate
- Nested Sampling with Normalising Flows for Gravitational-Wave Inference
- Importance nested sampling with normalising flows
- Costs of Bayesian Parameter Estimation in Third-Generation Gravitational Wave Detectors: an Assessment of Current Acceleration Methods
- Relative Binning and Fast Likelihood Evaluation for Gravitational Wave Parameter Estimation
- Distinguishing Kilonovae from Binary Neutron Star and Neutron Star-Black Hole Mergers
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