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arxiv: 2604.11381 · v1 · submitted 2026-04-13 · ⚛️ nucl-th · quant-ph

Improved quasiparticle nuclear Hamiltonians for quantum computing

Pith reviewed 2026-05-10 15:50 UTC · model grok-4.3

classification ⚛️ nucl-th quant-ph
keywords quasiparticle HamiltonianBrillouin-Wigner perturbation theorynuclear shell modelquantum computingopen-shell nucleisd shellHartree-Fock approximationeffective Hamiltonian
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The pith

Brillouin-Wigner perturbation theory refines quasiparticle Hamiltonians for open-shell nuclei to below 0.2 percent error against the shell model.

A machine-rendered reading of the paper's core claim, the machinery that carries it, and where it could break.

This paper shows how to extend a qubit-efficient quasiparticle encoding for nuclear Hamiltonians beyond semimagic cases. By applying Brillouin-Wigner perturbation theory, the description of open-shell nuclei in the sd shell reaches energy accuracies better than 0.2 percent relative to exact shell-model diagonalization. To keep the resulting effective Hamiltonian practical for quantum computers, a mean-field Hartree-Fock treatment replaces the non-quasiparticle part of the resolvent, yielding ground-state energies within 2 percent of the exact results. The work therefore provides a systematic route to accurate nuclear simulations on near-term quantum hardware without doubling the qubit count.

Core claim

We apply Brillouin-Wigner perturbation theory to systematically improve the quasiparticle description of open-shell nuclei in the sd shell, reaching an energy relative error below 0.2% compared to the nuclear shell model. Furthermore, to make the effective Hamiltonian suitable for quantum simulation, we introduce a mean-field Hartree-Fock approximation of the non-quasiparticle resolvent, achieving ground-state energies typically within 2% of the exact shell-model result. This represents a systematic improvement over the bare quasiparticle Hamiltonian while remaining within the reach of near-term quantum devices.

What carries the argument

The Brillouin-Wigner perturbation series applied to the quasiparticle pairing modes, together with the Hartree-Fock mean-field approximation to the resolvent that excludes quasiparticle excitations.

Load-bearing premise

The mean-field Hartree-Fock approximation of the non-quasiparticle resolvent remains accurate enough that the resulting effective Hamiltonian still captures the essential physics of open-shell nuclei while staying implementable on near-term quantum hardware.

What would settle it

Exact diagonalization of an open-shell sd-shell nucleus such as 28Si using the full Brillouin-Wigner effective Hamiltonian and finding that the Hartree-Fock approximated version deviates by more than 2% from the exact shell-model ground-state energy.

Figures

Figures reproduced from arXiv: 2604.11381 by Emanuele Costa, Javier Menendez.

Figure 1
Figure 1. Figure 1: FIG. 1. Schematic representation of the computational workflows for quasiparticle BW methods. [PITH_FULL_IMAGE:figures/full_fig_p004_1.png] view at source ↗
Figure 2
Figure 2. Figure 2: shows the residual relative error compared to the exact shell-model result, ∆re = (E∗ − Egs)/|Egs|, at convergence as a function of the total number of itera￾tions needed to reach convergence [PITH_FULL_IMAGE:figures/full_fig_p006_2.png] view at source ↗
Figure 4
Figure 4. Figure 4: compares the ground-state energy of the quasiparticle BW method with the exact HCI shell￾model exact result, via the relative error ∆re = (E∗ − Egs)/|Egs|. The orange circles show the results for the full BW approach, corresponding to [PITH_FULL_IMAGE:figures/full_fig_p007_4.png] view at source ↗
Figure 3
Figure 3. Figure 3: In contrast, neutron-rich nuclei such as [PITH_FULL_IMAGE:figures/full_fig_p007_3.png] view at source ↗
Figure 5
Figure 5. Figure 5: shows that the truncated HF BW method (black stars) has an average fidelity, F HF ≃ 0.88, with sizeable difference between nuclei, FHF ∈ [0.74, 0.97]. Naturally, the two nuclei with larger ∆re, 22Ne and 24Mg, show the lower fidelities, but also for 22S we find FHF < 0.85. In an isotope chain, FHF increases with neu￾tron number, where proton-neutron correlations become less relevant. Overall, the HF WB fide… view at source ↗
read the original abstract

Quantum computing is increasingly offering concrete solutions toward the simulation of nuclear structure, with the potential to overcome the exponential scaling that limits classical diagonalization methods in large spaces. A particularly efficient encoding scheme, based on collective like-nucleon pairing modes, reduces the qubit requirements by half and avoids the non-local operator strings of standard fermion-to-qubit mappings. While this quasiparticle framework provides accurate results for semimagic nuclei, it does not adequately describe open-shell systems where proton-neutron correlations become important. In this work, we apply Brillouin-Wigner perturbation theory to systematically improve the quasiparticle description of open-shell nuclei in the $sd$ shell, reaching an energy relative error below $0.2\%$ compared to the nuclear shell model. Furthermore, to make the effective Hamiltonian suitable for quantum simulation, we introduce a mean-field Hartree-Fock approximation of the non-quasiparticle resolvent, achieving ground-state energies typically within $2\%$ of the exact shell-model result. This represents a systematic improvement over the bare quasiparticle Hamiltonian while remaining within the reach of near-term quantum devices.

Editorial analysis

A structured set of objections, weighed in public.

Desk editor's note, referee report, simulated authors' rebuttal, and a circularity audit. Tearing a paper down is the easy half of reading it; the pith above is the substance, this is the friction.

Referee Report

2 major / 1 minor

Summary. The manuscript proposes improving quasiparticle nuclear Hamiltonians for quantum computing of open-shell nuclei by applying Brillouin-Wigner perturbation theory to incorporate proton-neutron correlations in the sd shell, claiming relative energy errors below 0.2% versus the nuclear shell model. It further replaces the exact non-quasiparticle resolvent with a mean-field Hartree-Fock approximation to ensure the effective Hamiltonian remains suitable for near-term quantum simulation, achieving ground-state energies typically within 2% of exact shell-model results.

Significance. If substantiated, the work would provide a systematic extension of pairing-mode quasiparticle encodings (which already halve qubit requirements) to open-shell systems while preserving hardware feasibility, addressing a clear limitation of prior quasiparticle approaches that are accurate only for semimagic nuclei.

major comments (2)
  1. [Abstract] Abstract: the central quantitative claims (relative error below 0.2% with Brillouin-Wigner perturbation theory and typically within 2% after the Hartree-Fock resolvent approximation) are stated without any accompanying numerical results, tables of energies for specific sd-shell nuclei, derivation steps, or error-bar analysis, so the robustness of the reported improvements cannot be assessed from the manuscript.
  2. [Resolvent approximation] The section introducing the mean-field Hartree-Fock approximation of the non-quasiparticle resolvent: this replacement is load-bearing for the quantum-simulability claim, yet no separate validation, error bound, or comparison isolating the effect of the approximation on pairing and collective correlations in open-shell nuclei is provided; the jump from <0.2% to ~2% error is noted but not analyzed.
minor comments (1)
  1. [Abstract] The abstract would be clearer if it specified the particular sd-shell nuclei or mass range for which the quoted error figures were obtained.

Simulated Author's Rebuttal

2 responses · 0 unresolved

We thank the referee for the careful and constructive review of our manuscript. We address each major comment below and will revise the paper accordingly to improve the presentation of results and validation of the approximation.

read point-by-point responses
  1. Referee: [Abstract] Abstract: the central quantitative claims (relative error below 0.2% with Brillouin-Wigner perturbation theory and typically within 2% after the Hartree-Fock resolvent approximation) are stated without any accompanying numerical results, tables of energies for specific sd-shell nuclei, derivation steps, or error-bar analysis, so the robustness of the reported improvements cannot be assessed from the manuscript.

    Authors: We agree that the abstract, as a concise overview, does not embed specific numerical tables or error bars. The full manuscript details the Brillouin-Wigner derivations in the methods section and presents numerical comparisons for multiple sd-shell nuclei in the results section. In revision we will (i) augment the abstract with one or two concrete examples (e.g., relative errors for ^{24}Mg and ^{28}Si), (ii) insert a compact summary table of ground-state energies, exact shell-model references, and relative errors, and (iii) add a short paragraph on the numerical error analysis already performed. These changes will make the quantitative claims directly verifiable from the revised manuscript. revision: yes

  2. Referee: [Resolvent approximation] The section introducing the mean-field Hartree-Fock approximation of the non-quasiparticle resolvent: this replacement is load-bearing for the quantum-simulability claim, yet no separate validation, error bound, or comparison isolating the effect of the approximation on pairing and collective correlations in open-shell nuclei is provided; the jump from <0.2% to ~2% error is noted but not analyzed.

    Authors: We acknowledge that an explicit isolation of the Hartree-Fock resolvent approximation is needed. In the revised manuscript we will add a new subsection that (a) compares ground-state energies obtained with the exact non-quasiparticle resolvent versus the Hartree-Fock approximation for representative open-shell nuclei, (b) quantifies the additional error introduced on pairing and quadrupole correlations, and (c) supplies a perturbative error bound consistent with the Brillouin-Wigner framework. This analysis will explain the observed increase from <0.2% to ~2% and directly support the claim that the approximated Hamiltonian remains suitable for near-term quantum simulation. revision: yes

Circularity Check

0 steps flagged

No circularity: derivation uses standard perturbation theory and mean-field approximation on prior quasiparticle basis

full rationale

The paper applies Brillouin-Wigner perturbation theory to improve an existing quasiparticle Hamiltonian for open-shell sd-shell nuclei and replaces the exact non-quasiparticle resolvent with a mean-field Hartree-Fock form to enable quantum simulation. These are conventional many-body techniques whose outputs are compared to independent shell-model benchmarks rather than being defined in terms of the target energies or fitted parameters. No equation reduces the final effective Hamiltonian or reported errors to the inputs by construction, and no load-bearing self-citation or uniqueness theorem is invoked in the provided text. The derivation chain remains self-contained against external validation.

Axiom & Free-Parameter Ledger

0 free parameters · 2 axioms · 0 invented entities

Review performed on abstract only; no explicit free parameters, new entities, or ad-hoc axioms are stated. The work inherits standard assumptions of the nuclear shell model and many-body perturbation theory.

axioms (2)
  • domain assumption The nuclear shell model supplies the exact reference energies for sd-shell nuclei
    Used as the benchmark against which relative errors are measured.
  • domain assumption Brillouin-Wigner perturbation theory is applicable to the quasiparticle Hamiltonian for open-shell systems
    Invoked as the systematic improvement method.

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