Open Access Article
Yibo
Chen
a,
Zirui
Sheng
b,
Weitang
Li
b,
Yong
Zhang
acd,
Xun
Xu
a,
Jun-Han
Huang
*a and
Yuxiang
Li
*cd
aState Key Laboratory of Genome and Multi-omics Technologies, BGI Research, Shenzhen, 518083, China. E-mail: huangjunhan@genomics.cn
bSchool of Science and Engineering, The Chinese University of Hong Kong, Shenzhen, Guangdong 518172, P.R.China
cBGI Research, Wuhan 430047, China. E-mail: liyuxiang@genomics.cn
dGuangdong Bigdata Engineering Technology Research Center for Life Sciences, BGI Research, Shenzhen 518083, China
First published on 21st January 2026
Accurate calculation of strongly correlated electronic systems requires proper treatment of both static and dynamic correlations, which remains challenging for conventional methods. To address this, we present VQE-PDFT, a quantum-classical hybrid framework that integrates the variational quantum eigensolver with multiconfiguration pair-density functional theory (MC-PDFT). This framework strategically employs quantum circuits for multiconfigurational wavefunction representation while utilizing density functionals for correlation energy evaluation. The hybrid strategy maintains accurate treatment of static and dynamic correlations while reducing quantum resource requirements compared to highly expressive quantum algorithms. Benchmark validation, performed via a noiseless quantum circuit simulator, on the charge-transfer dataset confirmed that VQE-PDFT achieved results comparable to conventional MC-PDFT. Building upon this, we developed shallow-depth hardware-efficient ansatz circuits and integrated them into a QM/MM multiscale architecture to enable applications in complex biological systems. This extended framework, when applied to electron transfer in the European robin cryptochrome protein ErCRY4 with noiseless simulations, yielded transfer rates that aligned well with experimental measurements. Finally, as a proof-of-concept hardware demonstration, we executed reduced-density-matrix measurements for a single protein conformation on a 13-qubit superconducting device and showed the impact of noise through a comprehensive error analysis.
From an electronic structure perspective, the challenge of evaluating strongly correlated systems lies in representing the multiconfigurational wavefunction.6 Addressing this problem has spurred the advent of several computational strategies, each with distinct advantages and limitations. Within the multiconfiguration self-consistent field (MCSCF) framework, complete active space configuration interaction (CASCI)7 provides a foundation by performing configuration interaction within a predefined active space. Building upon this foundation, the complete active space self-consistent-field (CASSCF) method enhances CASCI by simultaneously optimizing both the CI coefficients and orbital parameters, thereby more accurately capturing static correlation effects—the near-degeneracy effects arising from multiple electronic configurations of comparable energy.8,9
However, both CASCI and CASSCF often provide insufficient accuracy due to their incomplete treatment of dynamic correlation effects8,10—the instantaneous electron–electron repulsion effects.11 To remedy this deficiency, researchers have developed various post-SCF approaches that build upon MCSCF reference wavefunctions.12 Complete active space second-order perturbation theory (CASPT2)13,14 represents one of the most successful examples, systematically recovering dynamic correlation, though it suffers from computational scaling limitations.
To address these computational limitations, multiconfiguration pair-density functional theory (MC-PDFT)15,16 offers a promising alternative by combining CASSCF-derived density matrices with an on-top density functional that captures dynamic correlation through opposite-spin electron pair probabilities at identical spatial coordinates. This hybrid approach greatly improves computational scaling relative to traditional post-SCF methods.6,17
However, MC-PDFT''s efficiency remains fundamentally constrained by its underlying CASSCF calculation. The exponential scaling of CASSCF with active space size renders calculations for large chemical systems computationally prohibitive, even with state-of-the-art hardware and advanced approximation schemes.18
The emergence of quantum computing presents a potential solution to these exponential scaling challenges.19,20 Quantum algorithms naturally exploit superposition and entanglement to encode complex many-body wavefunctions, offering theoretical advantages for strongly correlated electronic systems.21 Meanwhile, current noisy intermediate-scale quantum (NISQ) devices have motivated the development of hybrid quantum-classical algorithms,22 most notably the variational quantum eigensolver (VQE)23 and its variants. These include ADAPT-VQE,24,25 which dynamically constructs quantum circuits through iterative operator selection; cluster-VQE,26 which reduces qubit requirements via system decomposition; DMET-ESVQE,27 which achieves the combined advantages of both circuit optimization and qubit reduction through a distinct embedding-based approach; and ansatz design to maintain physical symmetries including quantum-number-preserving constraints.28 Alternative frameworks such as quantum algorithms for density functional theory (DFT) have also been proposed.29
For large systems, spatial decomposition approaches offer a practical solution by partitioning the system into fragments amenable to quantum hardware. Recent methods combine fragment molecular orbital techniques with quantum embedding30 and utilize localized active space strategies to reduce quantum resource requirements through systematic treatment of inter-fragment correlations.31,32
Despite these advances, extending VQE-based methods to multiconfigurational systems remains problematic.33 Existing approaches such as UCCGSD, and k-UpCCGSD struggle with the simultaneous treatment of static and dynamic correlation,34,35 often requiring prohibitively deep quantum circuits that exceed current NISQ capabilities. Moreover, the qubit counts on near-term devices typically limit such ansatzes to compact active spaces, and dynamic correlation contributions from orbitals outside the active space remain missing. Besides, the inherent noise in NISQ devices raises fundamental questions about computational reliability36,37 for practical applications, necessitating error analysis in specific calculations. Therefore, the fundamental challenge lies in designing quantum algorithms that can efficiently capture multiconfigurational character while remaining compatible with near-term quantum hardware constraints.
An alternative paradigm leverages quantum devices to compute reduced density matrices (RDMs), delegating correlation energy recovery to classical post-processing. Notable implementations range from coupling self-consistent CASSCF with hardware-efficient sampling to mitigate measurement noise in small active spaces,38 to integrating VQE with adiabatic connection theory for systematic dynamic correlation recovery from orbitals outside the chosen active space.39 Furthermore, Boyn et al. developed a hybrid framework in which a quantum solution of the anti-Hermitian contracted Schrödinger equation directly yields N-representable 2-RDMs, which are then combined with multiconfiguration pair-density functional theory for classical correlation-energy evaluation.40
Collectively, the above RDM-based approaches support the viability of separating quantum wavefunction preparation from classical correlation recovery. Building upon this philosophy, we introduce a quantum–classical hybrid framework that integrates VQE with multiconfiguration pair-density functional theory (MC-PDFT), referred to as VQE-PDFT. This framework (described first below) then serves as the basis for two additional developments targeting realistic biological modeling and practical hardware execution.
First, at the methodological level, we employ VQE strictly as a CASCI solver to capture static correlation, while recovering additional dynamic correlation beyond the CASCI description via a classical MC-PDFT on-top functional. In this framework, the total energy is evaluated from a pair-density functional of CASCI-level RDMs rather than directly from the Hamiltonian expectation value, allowing the quantum computation in VQE-PDFT to be reduced to compact active spaces focused on static correlation. By contrast, bare-〈H〉 VQE approaches may access a comparable level of dynamic correlation by enlarging the active space mapped to qubits and/or employing highly expressive ansatzes (e.g., UCCGSD and k-UpCCGSD34,35), leading to increased qubit requirements and circuit depth.
Second, we embed VQE-PDFT within a multiscale quantum mechanics/molecular mechanics (QM/MM) workflow to study electron transfer in a cryptochrome, computing Marcus parameters and transfer rates from ensembles of protein conformations in a complex biological environment.
Third, we develop shallow, symmetry-preserving hardware-efficient ansatzes tailored to open- and closed-shell tryptophan active spaces of the cryptochrome electron-transfer center, further reducing qubit count and circuit depth to support an initial hardware demonstration.
In this study, we first validated VQE-PDFT on the CT7/04 Charge-Transfer benchmark dataset, confirming accuracy comparable to conventional MC-PDFT. We then presented its QM/MM application to electron transfer in the European robin cryptochrome protein (ErCRY4), where the transfer rates from noiseless simulations agreed well with ultrafast spectroscopy measurements.41 Finally, as a proof-of-principle hardware validation on a simplified active-space model, a single conformation experiment on a 13-qubit superconducting device illustrated feasibility on current NISQ hardware within well-defined resource limits.
Throughout this work, unless explicitly stated otherwise, most of the quantum circuit calculations were carried out on noiseless classical simulators in limited active spaces, with quantum hardware used only for a single proof-of-principle validation.
The modified workflow proceeds as follows: VQE optimizes a parameterized quantum circuit ansatz (UCCSD for the CT7/04 benchmark, and ROUCCSD or the empirical HEA circuits for the ErCRY4 application) to approximate the CASCI ground state in the chosen active space, from which one-particle and two-particle reduced density matrices (1-RDM and 2-RDM) are extracted by measuring the corresponding matrix element expectation values on the quantum circuit as shown in Fig. 1. These reduced density matrices are then utilized to compute the total energy following the MC-PDFT formalism.
The 1-RDM provides the kinetic energy T, nuclear–electron interaction Vne, total electron density ρ, and classical Coulomb repulsion Vee(ρ). The 2-RDM yields the on-top pair density Π, which combines with ρ to determine the on-top density functional energy Eot(ρ, Π) that captures exchange–correlation effects. Finally, together with the nuclear–nuclear repulsion Vnn, the total energy follows the standard MC-PDFT expression:
| E = T + Vne + Vnn + Vee(ρ) + Eot(ρ, Π). | (1) |
This hybrid strategy is more compatible with NISQ constraints because the quantum computation is confined to a CASCI active-space solver that captures static correlation, while dynamic correlation is recovered classically through the on-top functional.15 It therefore avoids treating both correlation regimes variationally on the quantum circuit, which would generally require a highly expressive yet prohibitively deep ansatz (e.g., UCCGSD34). Moreover, capturing a large part of the dynamic correlation beyond a compact active space would require an expanded orbital space, further increasing the qubit counts.
| Dimers | N q (dimer) | VQE | VQE-PDFT | MC-PDFT | W1-reference |
|---|---|---|---|---|---|
| NH3⋯FCl | 20 | 5.38 | 11.56 | 12.42 | 10.62 |
| NH3⋯Cl2 | 20 | 1.57 | 5.09 | 4.55 | 4.88 |
| NH3⋯F2 | 20 | −0.08 | 1.88 | 1.11 | 1.81 |
| HCN⋯FCl | 16 | 2.19 | 3.13 | 3.67 | 4.86 |
| H2O⋯FCl | 20 | 10.01 | 3.30 | 4.38 | 5.36 |
| C2H2⋯FCl | 20 | 4.13 | 3.07 | 4.01 | 3.81 |
| C2H4⋯F2 | 20 | −1.14 | 0.85 | 0.33 | 1.06 |
| MUE | 2.896 | 0.853 | 0.847 | — | |
This dataset comprises 7 dimers that exhibit significant charge transfer effects upon dissociation. These systems are notoriously difficult to calculate accurately due to two key factors: their inherent multiconfigurational character and the dramatic electronic reorganization that occurs during dissociation.43,44 Such characteristics make these dimers ideal test cases for evaluating multiconfigurational methods in further applications.16
Table 1 summarizes the CT7/04 dissociation energies obtained with CASCI-level VQE (‘VQE’), VQE-PDFT, and classical MC-PDFT, together with high-level Weizmann-1 theory reference values (‘W1-reference’).42 Utilizing the Unitary Coupled-Cluster Singles and Doubles (UCCSD) ansatz, our VQE-PDFT method achieved a mean unsigned error (MUE) of 0.853 kcal mol−1 relative to W1 theory, closely matching the classical MC-PDFT result of 0.847 kcal mol−1.16
We emphasize that this close agreement between VQE-PDFT and classical MC-PDFT for CT7/04 was achieved within the specific limited active spaces and numerical settings adopted here (SI Table S1), and different active-space choices or numerical approximations could modify the quantitative agreement even though both protocols share the same on-top functional.
Notably, for two dimers (NH3⋯F2 and C2H4⋯F2), the CASCI-level VQE (column ‘VQE’ in Table 1) yielded negative dissociation energies. This indicated that, within these active spaces, the bare CASCI-level energies could be insufficiently correlated for these charge-transfer interactions. When the identical VQE-derived 1- and 2-RDMs were instead combined with the MC-PDFT functional (VQE-PDFT column), the dissociation energies restored the correct sign and moved closer to the reference values, and the MUE was reduced to 0.853 kcal mol−1. This comparison implied that the improvement of VQE-PDFT over CASCI-level VQE arose primarily from the functional treatment of dynamic correlation, instead of a change in the underlying VQE state or additional quantum resources.
This interpretation is consistent with the analysis of Ghosh et al. for CT7/04, where classical CASSCF (an orbital-optimizing version of CASCI) was found to have the largest MUE (3.92 kcal mol−1) among the methods considered and yielded negative dissociation energies on C2H2⋯FCl and C2H4⋯F2 dimers in CT7/04. Ghosh et al. attributed this to the absence of an explicit approximation to the full dynamic correlation energy.16 Accordingly, the CASCI-level energies in the ‘VQE’ column may mainly reflect the known limitations of the CASCI framework with respect to dynamic correlation, rather than an intrinsic deficiency of the VQE algorithm itself. Conversely, the improved VQE-PDFT dissociation energies result from supplementing this missing dynamic correlation through the MC-PDFT functional applied to the same VQE-derived RDMs (even though the resulting energy is no longer a strict variational 〈Ψ|Ĥ|Ψ〉 for that state).
From this perspective, the ‘VQE’ column in Table 1 may be viewed as the CASCI-level analogue of the classical CASSCF reference step in conventional MC-PDFT, whereas the ‘VQE-PDFT’ and ‘MC-PDFT’ columns correspond to applying the same on-top pair-density functional to quantum- and classically obtained multiconfigurational references, respectively.
To better understand the error patterns, we further analyzed the deviations besides the MUE metric. The root-mean-square errors (RMSE) relative to the W1 reference were 1.129 kcal mol−1 for VQE-PDFT and 0.985 kcal mol−1 for MC-PDFT, showing that VQE-PDFT exhibited a slightly broader error distribution yet averaged out in the MUE metric. Additionally, inspection of the absolute total energies (SI Table S3) revealed a method-dependent systematic shift of VQE-PDFT compared to MC-PDFT results. However, since the dissociation energy is defined as an energy difference (Edimer − ∑Emonomer), these systematic shifts partially canceled out, leaving residual errors that were comparable to the classical MC-PDFT reference. This suggested that the agreement in dissociation energies reflects a combination of similar dynamic correlation treatments via the tPBE functional and the beneficial cancellation of systematic offset.
In summary, this benchmark suggests that VQE-PDFT may effectively describe the electronic correlation in these charge-transfer systems. This indicates its potential for handling similar complex interactions found in bio-molecules, where multiconfigurational character is ubiquitous. Moreover, the observation that method-dependent shifts partially canceled in energy differences provides the rationale for our subsequent application to the electron transfer process in ErCRY4 protein. Since the key parameters (reorganization energy and driving force in Marcus theory) are also defined as differences between single-point energies, we anticipate a similar degree of error cancellation, enabling reliable predictions of electron transfer rates even within simplified active-space models.
Overall, this framework addresses two key challenges: adapting a multiscale QM/MM architecture, based on standard electrostatic embedding and link-atom techniques, for complex biological environments; and designing hardware-efficient quantum circuits optimized for NISQ constraints in electron transfer calculations.
Regarding the multiscale coupling, the QM/MM machinery itself follows well-established practice. In our workflow, the quantum circuit is used specifically as a CASCI solver for the multiconfigurational QM region, replacing the classical CASSCF step within an otherwise MC-PDFT/QM/MM treatment. Because the present ErCRY4 proof-of-concept employs deliberately compact active spaces that are also classically tractable, we do not claim a demonstrated quantum speed-up for this application. Rather, the motivation is that, as qubit numbers and gate fidelities improve, a quantum CASCI solver could help alleviate the main bottleneck of classical multiconfigurational solvers, and thereby enable larger active spaces in the QM region within the same multiscale framework. This long-term perspective is consistent with quantum resource-estimate studies of other strongly correlated bioinorganic centers, such as the nitrogenase FeMo cofactor, where Fe–S clusters pose challenges for conventional multiconfigurational treatments and have been proposed as natural targets for future quantum simulations.3,48
![]() | ||
| Fig. 2 Multiscale calculation framework of ErCRY4 protein. The quantum mechanical (QM) region is set to be two indole rings on the adjacent tryptophan residues (TrpB and TrpC), which are treated in separate QM calculations, while the rest of the systems are considered at the molecular mechanical (MM) level. The standard electrostatic embedding and link-atom methodology are adopted for evaluating interactions between the QM and MM regions. The figures were drawn with the help of ChimeraX.47 | ||
Extending this architecture for the subsequent study, the standard electrostatic embedding and link-atom methodology are implemented to handle the interface between QM and MM regions. In particular, it involves capping the covalent ‘C–C’ bond cut at the QM/MM boundary, ensuring proper treatment of boundary effects.50
To provide a proof-of-concept application of this multiscale framework, we selected the electron transfer process between adjacent tryptophan residues (TrpB and TrpC in Fig. 2) in the European robin cryptochrome protein (ErCRY4) as our target study. This system presents an ideal test case due to its well-characterized experimental properties5,41 and the multiconfigurational nature. The electron transfer process involves photo-excitation of the FAD cofactor followed by sequential electron transfer among adjacent tryptophan residues, during which tryptophan residues alternate between neutral and cationic states.
In this QM/MM setup, the QM region is represented by two separated fragments corresponding to the indole rings of TrpB and TrpC. Each single-point QM calculation is carried out on one fragment (TrpB or TrpC), while the remainder of the amino-acid side chain is treated at the MM level. For each QM fragment, the VQE-PDFT calculations use a compact CASCI active space consisting of three frontier orbitals localized on the tryptophan indole ring (SI Fig. S1), with 4 or 3 active electrons for the neutral and cationic states, respectively. The corresponding CASCI Hamiltonian and active orbitals are generated by the CASCI module of PySCF51 as interfaced in TenCirChem,52 starting from Hartree–Fock canonical orbitals and using the default active-space construction based on the specified (Ne, No) pattern.
However, the cationic states exhibit open-shell electronic character with unpaired electrons, making the previously used standard UCCSD ansatz inadequate, as it assumes paired α and β electrons in each spatial orbital. This limitation, combined with NISQ device constraints, necessitates the development of specialized quantum circuits.
Our approach employs distinct quantum circuits for the two electronic states encountered in the transfer process: a closed-shell HEA (CHEA, Fig. 3A) for neutral tryptophan and an open-shell HEA (OHEA, Fig. 3B) for cationic tryptophan. Both circuits are empirically designed to maintain the particle number conservation for each spin (i.e., within the target Nα/Nβ symmetry sector after tapering), while achieving minimal circuit depth compared to the ROUCCSD ansatz. The design methodology is detailed in Section 4.2.
![]() | ||
| Fig. 3 The shallow-depth empirical ansatzes for electron transfer. (A) Closed-shell HEA circuit (CHEA) with a circuit depth of 4. (B) Open-shell HEA circuit (OHEA) with a circuit depth of 6. These two circuits are dramatically shallower than ROUCCSD with a circuit depth of 35. The circuit diagrams were drawn with the PennyLane library.53 | ||
To validate the accuracy of the empirical HEA circuits, we randomly extracted a protein conformation from ErCRY4 molecular dynamics simulations reported in ref. 5. We then applied our multiscale framework by defining two adjacent tryptophan residues as separated QM regions for computational analysis. We employed a systematic approach that generated eight single-point energy calculations for two tryptophan residues, encompassing four open-shell cationic states and four closed-shell neutral states. These states are typically encountered in electron transfer processes, and the specific procedure of constructing these states follows the four-point scheme54 (see also Section 2.4.2).
For this validation study, we performed calculations using three different methods: the empirical HEA, ROUCCSD, and full configuration interaction (FCI), each applied to the active space within the CASCI framework. The comparative results are presented in Table 2.
| E FCI | E ROUCCSD | E HEA | ΔEHEA-FCI | |
|---|---|---|---|---|
| 1 | −2.1968 | −2.1968 | −2.1947 | 0.0021 |
| 2 | −2.5535 | −2.5535 | −2.5500 | 0.0035 |
| 3 | −2.1902 | −2.1902 | −2.1899 | 0.0004 |
| 4 | −2.5424 | −2.5424 | −2.5391 | 0.0033 |
| 5 | −2.1912 | −2.1912 | −2.1899 | 0.0013 |
| 6 | −2.5621 | −2.5621 | −2.5584 | 0.0036 |
| 7 | −2.1963 | −2.1963 | −2.1958 | 0.0005 |
| 8 | −2.5310 | −2.5310 | −2.5279 | 0.0032 |
The results demonstrate that the proposed empirical HEA circuits achieve accuracy of energy differences typically ranging from 10−4 to 10−3 Hartree with respect to the FCI results. Moreover, ROUCCSD energies match FCI values within excellent precision (at least <10−4 Hartree). We note that this near identity between ROUCCSD and FCI may arise from the compact (3e, 3o) and (4e, 3o) active spaces adopted in this validation, and should not be interpreted as a general property of ROUCCSD for larger multiconfigurational active spaces, where it remains an approximate high-level reference to FCI.
Also in Table 2, one may observe the slightly smaller HEA-FCI deviations for the open-shell cases (rows 1, 3, 5, and 7), compared to closed-shell results. This is consistent with our deliberate circuit design: to accommodate the more complex open-shell configurations, OHEA is constructed with a modestly larger depth and more variational parameters than CHEA (depth 6 vs. 4, and 5 vs. 2 parameters; Fig. 3). At the same time, the empirical HEA circuits are intentionally constrained to a fixed shallow depth and a small number of variational parameters to prioritize NISQ feasibility. Therefore, the residual HEA-FCI discrepancies in Table 2 mainly reflect this resource-oriented ansatz choice rather than an intrinsic limitation of the general HEA framework.
Overall, this validation confirms that our HEA circuits maintain sufficient expressibility for the active space of the current electron transfer system while offering notable quantum resource savings.
![]() | (2) |
Our VQE-PDFT framework within the multiscale QM/MM architecture enables direct evaluation of the reorganization energy and driving force.
To quantify both the reorganization energy λ and driving force ΔGo, we employed the four-point scheme,54 a well-established thermodynamic approach that captures the essential physics of Marcus theory. This method is based on the fundamental assumption that the system responds instantaneously to changes in electronic charge distribution.55 This approximation, although it neglects potential non-Markovian effects arising from slower environmental responses,56 enables us to bypass costly dynamical simulations and focus directly on energetic differences between key electronic configurations.
As illustrated in Fig. 4, the four-point scheme evaluates single-point energies at four distinct state-geometry combinations: each electronic state (initial and final) calculated at both its own optimized nuclear conformation and at the geometry optimized for the other state. This approach captures the energetic penalty arising from the mismatch between optimal nuclear arrangements for different charge distributions. Thereafter, the reorganization energy and the driving force of a given protein conformation can be extracted through:
| ΔGo = |Eii − Eff|, | (3) |
| λ = |Eif − Eii| + |Efi − Eff|, | (4) |
To capture the dynamic behavior of the protein in biological environments, we sampled 20 distinct protein conformations from molecular dynamics simulations of ErCRY4 and applied the four-point scheme to each conformation using our VQE-PDFT/MM framework. We calculated λ and ΔGo using both ROUCCSD and the proposed empirical HEA circuits, obtaining averaged value of λ = 0.5701 eV and ΔGo = 0.0689 eV for ROUCCSD, and λ = 0.4356 eV and ΔGo = 0.0724 eV for HEA, as listed in Table 3 and detailed in the Supplementary Information. The good agreement between HEA and ROUCCSD results, considering the great reduction in circuit depth in HEA, validates the feasibility of the empirical HEA for the current biological application, achieving a balance between accuracy and quantum resource efficiency, although with a compact active space.
| Ansatz | λ | ΔGo | 〈|HDA|〉 | 〈|HDA|2〉 |
|---|---|---|---|---|
| ROUCCSD | 0.5701 | 0.0689 | 6.352 × 10−3 | 1.1431 × 10−4 |
| HEA | 0.4356 | 0.0724 |
We computed the 〈|HDA|〉 through transfer integral calculations between the TrpB and TrpC indole rings. The approach employed Boys localization57 to transform canonical molecular orbitals into spatially localized orbitals centered on individual tryptophan sites, enabling clear identification of the relevant frontier orbitals for each fragment. This localization procedure was essential for defining well-separated donor and acceptor orbitals in weakly coupled systems where standard canonical orbitals are typically delocalized across multiple sites.
The electronic coupling is extracted using the direct coupling (DC) scheme,58 which accounts for orbital non-orthogonality through:
| HDA = [TDA − (eD + eA)SDA/2]/(1 − SDA2), | (5) |
Applying this methodology to the same 20 protein configurations, we obtained an averaged electronic coupling of 〈|HDA|〉 = 6.35 × 10−3 eV (6.35 meV) that aligned well with the 5 meV reported by Timmer et al.,41 also listed in Table 3.
The computed rates were derived by substituting the averaged reorganization energies, driving forces, and electronic couplings into the Marcus expression (eqn (2)). As a result, our empirical HEA approach yielded kET = 0.944 × 1010 s−1, aligning well with both ROUCCSD calculations (0.864 × 1010 s−1) and the experimental ultrafast transient absorption measurements41 (0.709 × 1010 s−1), as shown in Fig. 5. Notably, these results were approximately one order of magnitude slower than previous DFT predictions5 ((5.0 ± 1.8) × 1010 s−1), as also pointed out in ref. 41.
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| Fig. 5 Electron transfer rate comparison. The red marked transfer rate was evaluated on quantum hardware. The single conformation results show rates one order of magnitude lower than the averaged values of 20 conformations, reflecting typical conformational fluctuations in MD simulations where tryptophan positioning variations can alter transfer rates by several orders of magnitude.56 The DFT prediction was obtained from ref. 5. Explicit parameters calculated for each conformation are listed in the SI. | ||
| Index | System | Empirical HEA on quantum hardware |
|---|---|---|
| 1 | point-a TrpB+ | −362.92966 |
| 2 | point-a TrpC0 | −363.17866 |
| 3 | point-b TrpB0 | −363.20554 |
| 4 | point-b TrpC+ | −362.91475 |
| 5 | point-c TrpB0 | −363.19954 |
| 6 | point-c TrpC+ | −362.91126 |
| 7 | point-d TrpB+ | −362.92451 |
| 8 | point-d TrpC0 | −363.18130 |
| λ | 0.47021 eV |
| ΔGo | 0.06764 eV |
| k ET | 2.61742 × 108 s−1 |
This result compared favorably with noiseless calculations: 1.89 × 108 s−1 (HEA) and 2.49 × 108 s−1 (ROUCCSD), demonstrating that quantum hardware may conduct electron transfer evaluations within a compact active space despite inherent noise. More explicit single-point energies and derived parameters are detailed in the Supplementary Information.
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| Fig. 6 Error analysis of single-point energies and Marcus parameters. ROUCCSD results are set as the comparison baseline. (A) Error comparison on 8 single-point energies of quantum hardware and noiseless empirical HEA, with quantum hardware results showing systematic errors (65.3 ± 14.2 mHartree positive deviation) compared to noiseless HEA relative to the ROUCCSD reference. The system indices follow the index column in Table 4. (B) Error distributions of quantum hardware and noiseless empirical HEA. (C) Error magnitude comparison between single-point energies and Marcus parameters. Explicit single-point calculations can be found in the Supplementary Information. | ||
This systematic bias indicated a non-random error source. The errors likely originated from correlated uncertainties in noisy matrix element measurements or from VQE-PDFT's systematic response to noisy RDMs, rather than from purely random quantum fluctuations.
Moreover, the systematic nature of these hardware errors is noteworthy for biological electron transfer applications. Unlike random noise that would propagate unpredictably and through energy difference calculations, systematic errors might enable partial cancellation when computing the energy differences that underlie Marcus theory parameters. This observation motivated examining how these correlated single-point energy errors influence the derived reorganization energy and driving force that determine electron transfer rates.
![]() | (6) |
This error cancellation effect was demonstrated in our calculations, as illustrated in Fig. 6B and C. While individual single-point energies exhibited errors of 61–86 mHartree on quantum hardware, the derived Marcus parameters showed notably reduced absolute uncertainties: λ differed from the ROUCCSD reference by 2.0 mHartree, and ΔGo by 0.9 mHartree. However, it should be noted that the relative errors of Marcus parameters actually increased due to their smaller absolute magnitudes (∼12% for λ, ∼36% for ΔGo).
Despite these relative error increases, the systematic nature of quantum hardware errors enables partial cancellation when computing energy differences. This error cancellation allowed the derived electron transfer rates (2.62 × 108 s−1) to achieve consistency with classical predictions (1.89 ∼ 2.49 × 108 s−1), demonstrating that the approach remains viable for the current electron transfer application. Additionally, together with the similar effect shown in the CT7/04 benchmark test, the observed error cancellation in energy differences may thus provide a strategic pathway for NISQ devices to contribute meaningfully to computational biochemistry, by focusing on difference-based observables rather than absolute electronic energies.
Validation on the CT7/04 dataset demonstrated excellent agreement with reference calculations (MUE = 0.853 kcal mol−1 with respect to W-1 theory), confirming the method's reliability for multiconfigurational systems. We also extended this framework to a biological electron transfer application by developing specialized hardware-efficient ansatz circuits optimized for NISQ device constraints, achieving circuit depths of 4–6, compared to 35 for ROUCCSD, while maintaining high accuracy.
Our comprehensive application to electron transfer in the European robin cryptochrome ErCRY4 protein yielded transfer rates (0.944 × 1010 s−1 for HEA and 0.864 × 1010 s−1 for ROUCCSD) that aligned well with experimental ultrafast spectroscopy measurements (0.709 × 1010 s−1), validating our quantum-classical approach for this complex biological environment. Finally, as a proof-of-concept hardware validation within this quantum-classical multiscale framework, we executed the reduced-density-matrix measurements for a single ErCRY4 protein conformation on a 13-qubit superconducting device and obtained an estimated electron transfer rate (2.62 × 108 s−1) that aligned well with noiseless simulations, even in the presence of hardware noise.
Moreover, this work also mitigates three challenges for NISQ-era quantum biology applications: explicit treatment of multiconfigurational electronic correlations through purpose-designed shallow-depth quantum circuits, enhancing the ability for calculating strongly correlated system; systematic error cancellation through focus on energy differences rather than absolute energies, where we discovered that errors partially cancel in Marcus parameter calculations with quantum hardware, alleviating the quantum noise's impact on derived observables; and integration within a scalable multiscale framework adaptable to future hardware improvements, minimizing software and algorithmic modification while maintaining utility via the flexible VQE calculation.
Several limitations warrant future investigation. Firstly, current quantum hardware constraints may restrict active space sizes and computational accuracy. Secondly, efficient optimization and measurement grouping methods should be developed to lower the costs of quantum computation, enabling sampling across more protein conformations on superconducting quantum hardware, which was the main obstacle while conducting experimental validation. Thirdly, our separate treatment of indole rings on two tryptophan residues, while justified by weak electronic coupling, represents an approximation that could be improved by simultaneous evaluation of multiple rings to capture longer-range interactions and intermediate transfer states. Besides, in this proof-of-principle study we did not perform a systematic sensitivity analysis with respect to the precise QM/MM partitioning or to enlarging the tryptophan active spaces, as such an investigation would require a substantially larger set of high-level quantum calculations; exploring these alternatives will be an important direction for future work.
Additionally, the empirical HEA circuits adopted here are constructed for the present compact tryptophan active spaces under fixed (Nα, Nβ) constraints and are not expected to be directly transferable. Therefore, developing more systematic and automated strategies for symmetry- and configuration-guided HEA constructions, and assessing their performance in larger active spaces and broader scenarios (e.g., bond-dissociation/potential-energy curves), would also be a valuable direction for future work.
Future developments will further focus on constraining electronic populations during VQE optimization through penalty functions or Lagrangian multipliers with information from Mulliken population analysis, enabling treatment of multiple simultaneous transfer pathways. As quantum hardware develops, our scalable framework can accommodate increased qubit counts and improved fidelities for more comprehensive biological system calculations.
In conclusion, VQE-PDFT illustrates a practical pathway for quantum computing applications in biochemistry, suggesting that despite current limitations, quantum-classical hybrid approaches may yield reasonably accurate predictions for simplified active-space models of particular biological processes and can serve as an initial step toward exploring quantum utility in molecular sciences.
| γpq = 〈ψ|a†paq|ψ〉, |
| γpq = 〈ψ(θ)|a†paq|ψ(θ)〉, |
| |ψ(θ)〉 = U(θ)|ψ0〉. |
This enables us to compute each element of 1-RDM by executing the circuit with frozen parameters and sampling the expectation value of the corresponding operators after fermion-to-qubit mapping such as the parity transformation.
The same procedure is also valid for computing 2-RDM Γpq,rs.
In this element-wise measurement protocol, the additional post-optimization measurement overhead is governed by the number of distinct RDM elements to be sampled. For an active space comprising Nso spin orbitals, the 1-RDM γpq and 2-RDM Γpq,rs would formally contain O(Nso2) and O(Nso4) matrix elements, respectively (up to constant prefactors from Hermiticity and index symmetries). After the fermion-to-qubit transformation, each fermionic operator is mapped to a constant number of Pauli words to be measured, so the number of distinct measurement operators required for sampling the full 1- and 2-RDM scales as O(Nso2) for the 1-RDM and O(Nso2) for the 2-RDM, respectively.
Given this measurement overhead, we note that alternative strategies have been proposed to reduce the quantum measurement cost of RDM evaluations. For instance, natural orbital functional (NOF) methods reconstruct an approximate 2-RDM from the measured 1-RDM, reducing formal sampling requirements from O(Nso4) to O(Nso2).60 However, because MC-PDFT depends explicitly on 2-RDM information through the on-top pair density Π, introducing an additional 2-RDM reconstruction approximation may bias the functional evaluation. Our approach therefore directly measures the 1-RDM and 2-RDM elements in the present work. Separately, for evaluating the CASCI energy one may further reduce measurement cost by truncating Pauli terms with small Hamiltonian coefficients. These term-selection techniques are complementary to VQE-PDFT and could be combined with our framework.
• Identify the active space and fermion-to-qubit mapping (parity transformation here), and determine the fixed Nα/Nβ symmetry sector;
• Reduce the qubit register by tapering qubits associated with these symmetries;
• Determine the set of computational-basis configurations that satisfy particle conservation;
• Construct a shallow symmetry-preserving circuit that couples these configurations with minimal depth and parameter count.
Owing to the strong particle-number constraints and the small, factorized structure of the α- and β-spin qubit registers in the present (4e, 3o)/(3e, 3o) cases, this iterative construction remains tractable and yields depth-4 (CHEA, Fig. 3A) and depth-6 (OHEA, Fig. 3B) circuits that are sufficiently flexible for the subsequent validation and hardware execution, compared to ROUCCSD's 35-layer requirement. A quantitative comparison of the logical circuit depths, total numbers of single- and two-qubit gates for ROUCCSD and the HEA circuits is provided in Supplementary Table S2(a).
This empirical approach represents a compromise necessitated by current NISQ limitations rather than fundamental algorithmic constraints that can be directly transferred for arbitrary systems. The system-specific ansatz optimized for tryptophan electronic structure patterns requires extensive reanalysis for different chemical environments or larger active spaces. For other systems, the same design workflow may be followed, but the resulting circuit structure will generally change with (a) the active-space size and occupation pattern (hence the number of qubits after symmetry tapering) and (b) the number and connectivity of dominant configurations within the target symmetry sector, which may require additional entangling layers and variational parameters to maintain accuracy. As quantum hardware develops to support deeper circuits (hundreds of circuit-depths) with high fidelity, more general approaches like ROUCCSD or highly expressive multi-layer HEAs may become preferable over these tailored solutions.61
(1) Pauli operator preparation. Pauli measurement operators were obtained through parity transformation of the corresponding matrix elements.
(2) Measurement grouping. Compatible measurement operators were grouped using a simple grouping strategy to reduce quantum measurement overhead and noise impact. For instance, operators Z1Z2I3I4 and I1I2Z3Z4 can be simultaneously measured using the single operation Z1Z2Z3Z4.
(3) Circuit compilation. The empirical HEA circuits and grouped measurements were uploaded to the quantum hardware platform. These circuits then underwent qubit mapping and gate decomposition to match the chip topology and native gate set. As shown in Fig. 7, the resulting compiled circuits utilized only 4 physical qubits, benefiting from our restrained use of two-qubit gates that eliminated the need for additional connectivity qubits. Quantitative information for the compiled HEA circuits on the 13-qubit device is summarized in SI Table S2(b).
(4) Circuit execution. Each compiled circuit was executed with 2048 measurement shots, returning raw bit-string distribution data.
(5) Readout error mitigation. Raw measurement data underwent readout error correction using the correlated Markovian noise model approach. This correction required calibration circuits executed once per single-point energy calculation with 8192 shots. The resulting calibration data were then stored for all subsequent measurements within that calculation. Finally, the error mitigation module processed raw bit-string distribution, calibration data, and target measurement operators to yield the corrected expectation value as the matrix elements.
(6) RDM assembly. Steps 1–5 were repeated for all required matrix elements to construct the entire 1-RDM and 2-RDM matrices.
This protocol enabled reliable extraction of reduced density matrices from noisy quantum hardware while maintaining computational efficiency through strategic measurement grouping and error mitigation.
Supplementary information (SI): visualizations of active space orbitals and detailed summaries of quantum resource requirements, including qubit counts and circuit depths for the computational schemes; tabulated data on absolute energies for the charge-transfer dataset, alongside calculated Gibbs free energies, reorganization energies, and electronic coupling values for the sampled protein conformations. See DOI: https://doi.org/10.1039/d5sc07528a.
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