Andrew Steiner Contact STEINERAW@ORNL.GOV All Publications Structure Factors for Hot Neutron Matter from Ab Initio Lattice Simulations with High-Fidelity Chiral Interactions Uncertainty quantification for neutrino opacities in core-collapse supernovae and neutron star mergers... Hot and dense matter equation of state probability distributions for astrophysical simulations Combining Electromagnetic and Gravitational-Wave Constraints on Neutron-Star Masses and Radii Detectability of neutrino-signal fluctuations induced by the hadron-quark phase transition in failing core-collapse supernova... Deducing neutron star equation of state from telescope spectra with machine-learning-derived likelihoods Deducing neutron star equation of state parameters directly from telescope spectra with uncertainty-aware machine learning From the microscopic to the macroscopic world: from nucleons to neutron stars Future prospects for constraining nuclear matter parameters with gravitational waves Hyperons and quarks in proto-neutron stars Tidal deformability with sharp phase transitions in binary neutron stars... Hot and dense homogeneous nucleonic matter constrained by observations, experiment, and theory Constraining nuclear matter parameters with GW170817 Nuclear Reactions in the Crusts of Accreting Neutron Stars The radius of the quiescent neutron star in the globular cluster M13 Testing the Formation Scenarios of Binary Neutron Star Systems with Measurements of the Neutron Star Moment of Inertia Constraining the mass and radius of neutron stars in globular clusters Constraining superfluidity in dense matter from the cooling of isolated neutron stars Cooling of neutron stars in soft x-ray transients White paper on nuclear astrophysics and low energy nuclear physics Part 1: Nuclear astrophysics... Reverse engineering nuclear properties from rare earth abundances in the r process The link between rare-earth peak formation and the astrophysical site of the r process... Neutron matter, symmetry energy and neutron stars Colloquium: Measuring the neutron star equation of state using x-ray timing... Neutron star radii, universal relations, and the role of prior distributions Pagination Current page 1 Page 2 Next page ›â¶Äº Last page Last » Key Links Organizations Physical Sciences Directorate Physics Division Fundamental Nuclear and Particle Physics Section Theoretical and Computational Physics Group
