Emulating <i>ab initio</i> computations of infinite nucleonic matter
W. G. Jiang, C. Forssén, T. Djärv, G. Hagen
Abstract
We construct efficient emulators for the computation of the infinite nuclear matter equation of state. These emulators are based on the subspace-projected coupled-cluster method for which we here develop a new algorithm called small-batch voting to eliminate spurious states that might appear when emulating quantum many-body methods based on a non-Hermitian Hamiltonian. The efficiency and accuracy of these emulators facilitate a rigorous statistical analysis within which we explore nuclear matter predictions for <a:math xmlns:a="http://www.w3.org/1998/Math/MathML"><a:mrow><a:mo>></a:mo><a:msup><a:mn>10</a:mn><a:mn>6</a:mn></a:msup></a:mrow></a:math> different parametrizations of a chiral interaction model with explicit <b:math xmlns:b="http://www.w3.org/1998/Math/MathML"><b:mi mathvariant="normal">Δ</b:mi></b:math>-isobars at next-to-next-to leading order. Constrained by nucleon-nucleon scattering phase shifts and bound-state observables of light nuclei up to <d:math xmlns:d="http://www.w3.org/1998/Math/MathML"><d:mmultiscripts><d:mi>He</d:mi><d:mprescripts/><d:none/><d:mn>4</d:mn></d:mmultiscripts></d:math>, we use history matching to identify nonimplausible domains for the low-energy coupling constants of the chiral interaction. Within these domains we perform a Bayesian analysis using sampling and importance resampling with different likelihood calibrations and study correlations between interaction parameters, calibration observables in light nuclei, and nuclear matter saturation properties. Published by the American Physical Society 2024