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Tom Plies

Publications and source records attributed to Tom Plies.

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Active-subspace learning reveals dominant parameter directions in nuclear observables

Nuclear observables computed using ab initio methods can depend on many low-energy constants (LECs) of the underlying chiral effective field theory interactions, while being sensitive to only a few LEC combinations. We use active-subspace learning to identify these dominant parameter directions directly from many-body calculations. For ground-state energies and charge radii of oxygen isotopes, we find that more than 99% of the gradient-based variation is concentrated along a single direction for each observable in the 17-dimensional LEC space. Comparing these directions across nuclei and observables quantifies similarities in their LEC dependence. The same analysis yields derivative-based global sensitivities without requiring a global emulator. Active-subspace directions can also serve as an efficient representation for emulation, greatly improving Gaussian-process emulators especially for broad LEC variations. We demonstrate this for Hartree-Fock calculations of $^{48}\mathrm{Ca}$, where the emulator error is improved with active-subspace learning by more than two orders of magnitude.

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Uncertainties with low-resolution nuclear forces

Low-resolution nuclear Hamiltonians, obtained from chiral effective field theory (EFT) and softened using renormalization group techniques, have been very successful in nuclear structure theory. The associated EFT truncation uncertainty for these potentials is difficult to quantify. We use singular value decompositions of low-resolution nuclear forces to obtain an operator basis to study Hamiltonian uncertainties for these potentials. We perform Bayesian inference for the singular values and three-body low-energy constants, the free parameters of nuclear Hamiltonians in our framework, using likelihoods based on nucleon-nucleon phase shifts and triton observables to account for the EFT truncation uncertainties in these quantities. Validating our inference, we find good reproduction of input uncertainties for low-energy phase shifts and three-nucleon observables. On the other hand, uncertainties for higher-energy phase shifts are systematically underestimated, which we attribute to limitations of the singular value decomposition and neglected correlations between phase shifts at different energies. We propagate the resulting distribution of Hamiltonians forward to predictions for ground-state properties of $^{24,28}$O and $^{48}$Ca, comparing against other state-of-the-art nuclear structure predictions. Our approach makes it possible to account for EFT uncertainties when using low-resolution potentials, which is important for many ongoing studies in exotic nuclei.

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