Set Transformer inference of the neutron star equation of state from stellar observations
nucl-th, astro-ph.HE, hep-ph
Submitted: 2026-09-25
Updated: 2026-09-25
Terminology
Sources
- Constraining neutron star tidal Love numbers with gravitational wave detectors
- Upper limit set by causality on the tidal deformability of a neutron star
- Refined Mass and Geometric Measurements of the High-Mass PSR J0740+6620
- A NICER view of PSR J1614 - 2230: a massive and compact millisecond pulsar
- Properties of the binary neutron star merger GW170817
- Dense matter with eXTP
- STROBE-X: X-ray Timing and Spectroscopy on Dynamical Timescales from Microseconds to Years
- Probing the neutron star interior and the Equation of State of cold dense matter with the SKA
- Non-parametric inference of the neutron star equation of state from gravitational wave observations
- Nonparametric Inference of Neutron Star Composition, Equation of State, and Maximum Mass with GW170817
- Nonparametric constraints on neutron star matter with existing and upcoming gravitational wave and pulsar observations
- Extracting nuclear matter properties from the neutron star matter equation of state using deep neural networks
- Mapping neutron star data to the equation of state using the deep neural network
- Neural network reconstruction of the dense matter equation of state from neutron star observables
- Decoding Neutron Star Observations: Revealing Composition through Bayesian Neural Networks
- From NS observations to nuclear matter properties: a machine learning approach
- Reconstructing the neutron star equation of state from observational data via automatic differentiation
- A Physics Informed Bayesian Neural Network for the Neutron Star Equation of State
- Neural Simulation-Based Inference of the Neutron Star Equation of State directly from Telescope Spectra
- Conditional variational autoencoder inference of neutron star equation of state from astrophysical observations
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