Quantifying uncertainties and correlations in the nuclear-matter equation of state
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In this paper, the size and smoothness properties of the correlated EFT truncation error were extracted from high-order many-body perturbation theory calculations with nucleon-nucleon and three-Nucleon interactions up to fourth order in the chiral effective field theory.Abstract:
We perform statistically rigorous uncertainty quantification (UQ) for chiral effective field theory ($\ensuremath{\chi}\mathrm{EFT}$) applied to infinite nuclear matter up to twice nuclear saturation density. The equation of state (EOS) is based on high-order many-body perturbation theory calculations with nucleon-nucleon and three-nucleon interactions up to fourth order in the $\ensuremath{\chi}\mathrm{EFT}$ expansion. From these calculations our newly developed Bayesian machine-learning approach extracts the size and smoothness properties of the correlated EFT truncation error. We then propose a novel extension that uses multitask machine learning to reveal correlations between the EOS at different proton fractions. The inferred in-medium $\ensuremath{\chi}\mathrm{EFT}$ breakdown scale in pure neutron matter and symmetric nuclear matter is consistent with that from free-space nucleon-nucleon scattering. These significant advances allow us to provide posterior distributions for the nuclear saturation point and propagate theoretical uncertainties to derived quantities: the pressure and incompressibility of symmetric nuclear matter, the nuclear symmetry energy, and its derivative. Our results, which are validated by statistical diagnostics, demonstrate that an understanding of truncation-error correlations between different densities and different observables is crucial for reliable UQ. The methods developed here are publicly available as annotated Jupyter notebooks.read more
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How Well Do We Know the Neutron-Matter Equation of State at the Densities Inside Neutron Stars? A Bayesian Approach with Correlated Uncertainties.
TL;DR: This work introduces a new framework for quantifying correlated uncertainties of the infinite-matter equation of state derived from chiral effective field theory (χEFT), and produces the first statistically robust uncertainty estimates for key quantities of neutron stars.
Journal ArticleDOI
Neutron-star tidal deformability and equation-of-state constraints
TL;DR: In this article, the role of the tidal deformation in observations of coalescing neutron stars with gravitational waves was discussed and how it can be used to probe the internal structure of Nature's most compact matter objects.
Journal ArticleDOI
GW190814: Impact of a 2.6 solar mass neutron star on the nucleonic equations of state
TL;DR: In this paper, Covariant density functional theory was used to investigate the properties of finite nuclei and neutron stars, while enforcing causality at all densities, and it was shown that the stiffening of the equation of state required to support supermassive neutron stars is inconsistent with either constraints obtained from energetic heavy-ion collisions or from the low deformability of medium-mass stars.
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