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Second-Order Perturbation Theory in Continuum Quantum Monte Carlo Calculations

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arxiv 2302.07285 v2 pith:7X3AQSXJ submitted 2023-02-14 nucl-th cond-mat.quant-gasphysics.comp-ph

Second-Order Perturbation Theory in Continuum Quantum Monte Carlo Calculations

classification nucl-th cond-mat.quant-gasphysics.comp-ph
keywords many-bodynuclearsecond-ordercarloenergymonteordertheory
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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We report on the first results for the second-order perturbation theory correction to the ground-state energy of a nuclear many-body system in a continuum quantum Monte Carlo calculation. Second-order (and higher) perturbative corrections are notoriously difficult to compute in most ab initio many-body methods, where the focus is usually on obtaining the ground-state energy. By mapping our calculation of the second-order energy correction to an evolution in imaginary time using the diffusion Monte Carlo method, we are able to calculate these nuclear corrections for the first time. After benchmarking our method in the few-body sector, we explore the effect of charge-independence-breaking terms in the nuclear Hamiltonian. We then employ that approach to investigate the many-body, perturbative, order-by-order convergence that is fundamental in modern theories of the nucleon-nucleon interaction derived from chiral effective field theory. We find cutoff-dependent perturbativeness between potentials at higher chiral order and also that the difference between leading order and next-to-leading order potentials is nonperturbative; both of these results have important implications for future nuclear many-body calculations. Our approach is quite general and promises to be of wide applicability.

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Cited by 2 Pith papers

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  1. Quantum Monte Carlo calculation of $\delta_C$ in the superallowed beta decay of $^{10}$C

    nucl-th 2026-05 unverdicted novelty 6.0

    Ab initio QMC calculations yield δ_C ≈ 0.15–0.25% for ¹⁰C superallowed beta decay, consistent across phenomenological and chiral interactions within 34–65% relative uncertainties.

  2. Perturbative calculations of light nuclei up to N$^3$LO in chiral effective field theory

    nucl-th 2026-04 unverdicted novelty 5.0

    Perturbative N3LO calculations in chiral EFT with RG-guided power counting yield robust predictions for light nuclei energies when calibrated on the tritium binding energy.