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Bridging Quantum Mechanics and Biology at the Million-Atom Scale
Open accessPreprint — published as 10.1038/s42004-026-02038-y
Abstract
Quantum-mechanical simulations provide the most fundamental description of matter, yet their computational cost has limited applications to systems containing at most thousands of atoms. Here, we present an all-electron quantum-mechanical framework that extends the accessible system size to the multimillion-atom regime. By combining an algorithmically optimized Hartree-Fock formalism with divide-and-conquer, our new approach efficiently handles structures containing millions of atoms with subatomic resolution. We demonstrate this approach on very large biological systems, including a complete bacteriophage in water, totalling over 150 million electrons, representing, to our knowledge, the largest quantum-mechanical calculation performed to date. Our framework allows computing spectral data for DNA and drugs and enables protein structure assessments in strong agreement with structure evaluations by AlphaFold. This approach opens new avenues in quantum physics, structural biology, spectroscopy, bioinformatics, medicine, and materials science.
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![Figure 4: Comparison of quantum-mechanical atomic energies with AlphaFold confidence scores. Atomic energies from Hartree–Fock calculations are compared with AlphaFold’s pLDDT score for three predicted protein structures: Evasin P1126 (PDB AF_AFA0A023FF81F1) (a), MHC Class II Beta Chain (AF_AFA0A023IKK2F1) (b) and Friend of Echinoid, Isoform H (AF_AFA0A023GPK8F1) (c). For each protein, the left column shows ribbon diagrams and non-hydrogen atoms. The middle column (b,e,h) displays atomic energies computed in a solvated environment (10 Å water shell), smoothened using a Savitzky–Golay filter, scaled by element number, and linearly rescaled to match the pLDDT range. The right column (c,f,i) shows the corresponding AlphaFold pLDDT scores mapped onto atoms. Energies of outlier atoms were clipped to match the [0,100] range of pLDDT values. Protein structures in a, d and g were visualized using ChimeraX19. Data from rcsb.org42.](/paper-figures/c25b3e07381b469cb90da170a331781d/bridging-quantum-mechanics-and-biology-at-the-million-atom-scale-figure-4.jpg)
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Highly accurate protein structure prediction with AlphaFold
Jumper, J., Evans, R., Pritzel, A., Green, T., Figurnov, M., Ronneberger, O., Tunyasuvunakool, K., Bates, R., Žídek, A., Potapenko, A., et al. (2021) · Nature · doi:10.1038/s41586-021-03819-2 · Cited by 43,764
AlphaFold and Implications for Intrinsically Disordered Proteins
Ruff, K. M., & Pappu, R. V. (2021) · Journal of Molecular Biology · doi:10.1016/j.jmb.2021.167208 · Cited by 635
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- 47. Rackers, J. A., Tecot, L., Geiger, M., & Smidt, T. E. (2023). A recipe for cracking the quantum scaling limit with machine learned electron densities. Machine Learning: Science and Technology, 4(1), 015027. Methods Modifications to the Hartree–Fock algorithm Unlike density functional theory (DFT), Hartree–Fock is a wavefunction-based method and does not directly operate on the electronic density. Each electronic interaction integral contains products of four wave functions. As the system grows, the amount of involved wave functions increases, and the number of electronic repulsion integrals (ERIs) scales with the fourth power of the system size, making their evaluation one of the main computational bottlenecks of Hartree–Fock calculations. To address this, we introduce systematic approximations that significantly reduce the computational effort. Both wavefunction-wavefunction30 and density-density interactions are truncated using physically motivated thresholds. Since wave functions decay exponentially with distance, only nearby orbitals contribute significantly to overlaps (see subsection “Density cut-offs”). We assess the relevance of a density by calculating the overlap of its two constituent wave functions. For orbital types with negative signs, we use the absolute of the product to capture significant interactions that may otherwise cancel numerically but still produce meaningful contributions, especially to energy gradients, which are important for force calculations. Once densities below the threshold are excluded, the scaling of ERI evaluations drops from quartic to quadratic. To further reduce complexity to linear scaling (order N), we introduce a cut-off for the Coulomb interaction based on inter-density distance (see subsection “Coulomb cut-offs”). Since electrostatic interactions decay with the inverse of the distance between two charges, we use a Coulomb cut-off between 8 and 12 Å, similar to that employed in classical forces fields for biophysical simulations. The distance of two densities is defined as the distance between the centres of the two wavefunction pairs that generate them. Only ERIs with Coulomb distances below the Coulomb cut-off are calculated. For ERIs with distances near the cut-off, we apply a smoothening function to ensure continuity. An ERI is evaluated if the overlap threshold of both densities is exceeded and their centres lie within the Coulomb cut-off. Additionally, we compute the product of the two density relevance values (see the next subsections), divide it by the distance between their centres, and compare it to a final relevance threshold. This avoids evaluating interactions between weakly overlapping densities and/or those separated by large distances. To further accelerate the process, we adopt an efficient and parallelizable ERI algorithm48,49,50 based on the so-called Gaussian lobe functions32,51 (see subsection “Basis function fitting”). Unlike conventional approaches52,53,54,55, which use angular prefactors (x, y, z) to construct directional orbitals, our method builds positive and negative lobes from distinct Gaussian components. This removes angular dependencies and simplifies the integral expressions, making them uniform across orbital types. As a result, all ERI calculations can be performed by using the same expression, which enables a simple parallelisation for both ERIs and their derivatives (necessary to calculate atomic forces). We also precompute components of the ERIs which only depend on pairs of wave functions. This reduces the full calculation of the electronic repulsion between two densities consisting of in total of four Gaussian functions to only 6 additions, 8 multiplications, 10 memory accesses, 1 square root and the evaluation of the error function (see below). For most interactions with large separations, the error function can be approximated as unity, further reducing computational cost. The following subsections detail the generation of the lobe-based basis functions, the calculation of the density relevance, the calculation of the Coulomb interaction relevance and the mathematical expressions for the modified ERI algorithm. Basis function fitting In electronic structure calculations, wave functions are commonly modelled as Slater-type orbitals (STOs), which for an s-orbital have the form. To enable efficient integration, STOs are typically approximated by using Gaussian functions of the form. Each STO is approximated by a linear combination of Gaussians as This approximation enables an analytic evaluation of key integrals52,53,54,55, relevant for the overlap matrix, the kinetic and nuclei energy as well as the Coulomb and exchange interaction of the electrons in the system. Orbitals with higher angular momenta are typically expressed via Gaussians containing cartesian prefactors (). Although these integrals can also be evaluated analytically, their complexity increases due to the recursive nature of the associated expressions52,53,54,55. Furthermore, different angular momentum combinations require distinct equations, reducing parallelisation efficiency. To avoid this bottleneck, we here adopt Gaussian lobe function expansions32,51, which allow the construction of basis sets without cartesian prefactors. We show in this work that this approach, though currently not widely used, is particularly well-suited to modern computing architectures optimized for high parallelisation. It also enables the evaluation of ERIs using a unified matrix formalism, which is potentially compatible with GPU acceleration56. The algorithms for ERI evaluation are described in the section “Electron repulsion integral algorithm”. For fitting, we start with a Slater-type orbital of the STO-6G type taken from the Basis Set Exchange57. In the case of p-orbitals, we approximate them with 6 Gaussian functions, three paced symmetrically slightly to the left and three to the right of the orbital centre. This corresponds in accuracy to a conventional STO-3G orbital. The fitting is performed on a three-dimensional real space grid. Fit parameters include 3 contraction exponents and 3 coefficients, with the latter multiplied by on one side to model the nodal character of p-orbitals. For the optimisation of the parameters during the fitting process, the trust region algorithm is used. This is done via the function curve_fit from the mathematic Python library scipy58. Density cut-offs A density is defined as the product of two wave functions: To determine whether a given density is relevant for further calculations, we compute a scalar value given by the integral over the absolute value of all pairwise products of Gaussian functions: This equation is valid for s-type orbitals, where the integrand remains positive. Orbitals with nonzero angular momentum (e.g. p-orbitals) include prefactors which would require using the absolute values to ensure that the integrand is always positive. However, using these absolute values makes an analytic evaluation of the overlap integrals impossible. To resolve this, we developed an approach to represent each lobe of orbitals with a separate set of Gaussians. The previously described lobe-based basis functions (which achieve a nodal plane by summing Gaussians of different signs) are not suitable here, as their absolute-value integrals do not correspond to the absolute value of the full orbital. Instead, we independently fit each lobe of a p-type orbital using Gaussian functions, and then reconstruct the full orbital by combining lobes with different signs and different centres. The representation of a p-type orbital used for the density relevance calculations is given by: where is the sign of lobe and each cartesian direction has an individual contraction factor (e.g. ) and offset (e.g. ) for higher flexibility upon fitting. The fitting process is identical to that described in the section “Basis function fitting”. Coulomb cut-offs In the Hartree–Fock formalism, the Coulomb interaction is modelled as the repulsion between two electronic densities. Following the method described above, Coulomb interactions are neglected if the separation between densities exceeds a defined cut-off. However, since densities are not point-like, a suitable distance metric must be established to estimate their effective separation. For this purpose, each density is assigned an origin, calculated as the arithmetic mean of the atomic positions associated with the two basis functions forming that density. The interaction distance between two densities and is defined as: where are the positions of the atoms involved in the four basis functions. A lower and upper cut-off threshold and (typically 8 and 10 Å), are introduced to control the inclusion of interactions. For density pairs with distances between these two thresholds, a smooth transition is applied using a cut-off function to avoid discontinuities. The scaling function (cut-off function) used is which smoothly interpolates between 1 and 0 as increases in the interval The distance interval is linearly mapped to the domain of. Electron repulsion integral algorithm An electron repulsion integral (ERI) describes the interaction between two electronic densities: where each orbital is expanded in terms of Gaussian functions. Each ERI of the individual Gaussian functions is given by: with the confluent hypergeometric function, two overlaps and, a factor and a distance which are defined as: We define and evaluate the confluent hypergeometric function using the following equation: where the error function can be efficiently approximated using: (with coefficients, ,, , and )59. For large the error function rapidly approaches 1, since and, and can be approximated accordingly. We recall that we evaluate the ERIs of the form It will only be necessary to compute a small part of all possible combinations, since we use both a density cut-off and a Coulomb cut-off. Therefore, and to reduce redundant computation, the quadruple summation over all Gaussians is reformulated as a double summation over precomputed Gaussian pairs and, for which the quantities and as well as and, respectively, are stored in lookup tables. This is practical because number of density pairs is considerably smaller than the total number of ERIs. The complete ERI evaluation algorithm can be visualized in terms of a three-dimensional tensor: the first and second axis are the sums described above and the third axis is the list of all relevant combinations. Summing up this tensor along the first two axes yields the full list of ERIs. It must be noted that each integral in this tensor is computed by using the same equation. However, the lengths of the first two axes and are not always the same as the number of used Gaussian functions is not the same for all wave functions. To account for this, we modify the equation for by setting the limits of the sums to and which leads to: where is if and —otherwise it is. Therefore, describes if the index combination is defined for the set of Gaussian functions within. This method allows the evaluation of all with the same equation and is therefore highly parallelizable. Additionally, it saves memory, since no intermediate values are stored (all Gaussian ERIs become contracted immediately in each step of the loop over. Precomputing and storing intermediate values dependent on only one density (,, and ) reduce the computational effort as well. Validation of cut-offs and basis To ensure that the proposed cut-off methods and basis function manipulations do not significantly compromise the accuracy of the calculations, results were benchmarked against the quantum-chemistry package ORCA13,60,61,62,63,64. Specifically, we assessed the agreement between our results and a standard calculation using the STO-3G basis set, focusing on both total and orbital energies. This allowed us to quantify the impact of lobe function expansion and interaction truncations on the computed energies. As a test system, we selected the molecule beta-carotene (C40H56), which involves 541,089,856 unique ERIs, of which 30,572,290 were considered to have relevant density contributions. Among these, 3,946,243 integrals met both density and Coulomb interaction relevance criteria. The total electronic energy calculated using our implementation was − 1528.547 Hartree (Ha), compared with − 1528.663 Ha obtained via ORCA. This corresponds to an absolute deviation of 0.115 Ha, or 0.0075%. For the orbital energies, we compared all valence orbitals and the ten lowest virtual orbitals, yielding a root mean square deviation of 7.98 mHa. Using only the Coulomb cut-off leads to a value of 7.57 mHa, whereas only density cut-offs result in an error of 6.07 mHa. No cut-offs at all result in a deviation of 3.23 mHa which is attributed to the modified basis functions in the lobe function expansion which do not match the STO-3G basis exactly and therefore lead to a small error. In terms of computational performance, ORCA required 192 seconds for a beta-carotene calculation on an Intel i5 processor. In comparison, our implementation with all cut-offs was completed in 21 seconds. When disabling the Coulomb cut-off and using a minimal density threshold of 10− 10, typical of many Hartree–Fock codes, the runtime increased to 131 seconds. The accuracy of subsystem splitting was tested using the protein Evasin P1126 (PDB ID: AF_AFA0A023FF81F1)42. For atomic energy calculations, only valence electrons were considered. Subsystems were constructed by segmenting the amino acid chain of the whole protein into smaller peptide fragments. Comparing a full Hartree-Fock calculation with the subsystem-based approach, we obtained a root mean square deviation of 0.385 Ha for the atomic energies, corresponding to a relative error of 0.444%. Parallel Hartree–Fock on large systems The density cut-off was set to 10− 4 and the Coulomb cut-off to 10 Å with a smooth transition to zero starting at 8 Å. The self-consistent cycle of the Hartree–Fock calculation used a convergence threshold of 10− 6 for the RMSD of the density matrices. The STO-3G basis set was split into individual Gaussian functions to allow an ERI evaluation according to the above-mentioned Gaussian lobe function expansion algorithm. System preparation involved solvation in water using the solvation tool of the programme Visual Molecular Dynamics (VMD)65. The solvated system was then partitioned into subsystems on a 3D mesh. Hartree-Fock calculations were carried out independently for each subsystem. To reconstruct the total electronic density, the density matrix elements were chosen from the subsystem containing both atoms corresponding to the two basis functions. If the basis functions were associated with different subsystems, the mean of the relevant density matrix elements was used. The total electronic density was then calculated as where is the total number of basis functions, is a relevance determining whether the pair basis functions and contributes significantly, and is the corresponding element of the density matrix. Spectral calculation parameters For the quantum spectral calculations, we employed the real-time time-dependent Hartree–Fock (RT-TDHF) formalism, as it scales more favourably for larger systems than the linear-response time-dependent Hartree–Fock (LR-TDHF) approach, which theoretically scales with the sixth power of the system size. In RT-TDHF the system is excited by an electric field pulse and propagated in time using quantum-mechanical time evolution. During the propagation, the dipole moments are recorded at each time step, and the frequency-dependent polarizability and absorption spectra are obtained via discrete Fourier transform of the dipole time series. The systems were propagated over 2,000 steps with a time step of 0.25 atomic units (a.u.), corresponding to a total propagation time of 500 a.u. (12.1 fs). The applied electric field pulse had a strength of 10− 5 a.u., a standard deviation of 0.2 a.u., and a starting time of 2 a.u. During the Fourier transform, an attenuation factor of 0.01 a.u. was used to supress numerical noise. Following established practice, the resulting spectra were rescaled66,67 to account for the systematic shifts in excitation energies inherent to time-dependent Hartree–Fock and density functional theory calculations. A rescaling factor of 1.335 was applied, consistent with the benchmark study by Jacquemin et al., who computed TDHF spectra for a wide range of organic dyes67. Atomic energy processing The atomic energies used for the comparison with AlphaFold’s pLDDT scores were smoothed using a Savitzky-Golay filter68 with a window length of 150. To match the scale of pLDDT values, the computed energies were multiplied by the factor of 15 and shifted by a structure-specific offset (–430, − 440 and − 460 for PDB entries AF_AFA0A023FF81F142, PDB AF_AFA0A023IKK2F142 and AF_AFA0A023GPK8F142, respectively). The rescaled energies were truncated at the corresponding structure’s maximum and minimum pLDDT values to eliminate extreme atomic energy outliers. A modified expression for atomic energies was employed, defined as where is the atomic energy of atom, is the atomic charge (used for normalisation), is the number valence basis functions for atom (excluding core contributions), and is the total number of basis functions., and denote the density matrix, core Hamiltonian, and two-electron interaction matrix elements, respectively. System preparation was based on the aforementioned PDB entries42, with solvation performed using a 10 Å water shell generated via the solvation tool of Chimera69. Programme implementation The described programme is written in the Python programming language70. To achieve high computational performance, all computational demanding functions are written either in matrix form or compiled to machine code with just-in-time (JIT) compilation. For JIT compilation, the library Numba71 was used, and matrix operations were performed with Numpy72 or PyTorch73. Visualisation of results and plotting were performed using the library Matplotlib74. Biomolecular structures and visualisation All calculations in this article were based on biomolecular structures obtained from the RCSB Protein Data Bank (PDB)42. The structures and their full references (including original research articles and PDB entries) are as follows: PDB 2M3X28 (12-bladed propeller protein), PDB 1H6831,75 (rhodopsin), PDB 6Q3G1,76 (bacteriophage P68), PDB 1A7Y5,77 (Actinomycin D), PDB 1D793,78 (DNA with 8 base pairs), PDB 2JYK4,79 (DNA with 21 base pairs), PDB 1MNV6,80 (Actinomycin D bound to DNA), PDB 8WL233,81 (flagellar motor), PDB 7PKR34,82 (vault protein complex). Structures used for comparing AlphaFold’s pLDDT scores to atomic energies include: PDB AF_AFA0A023FF81F1 (Evasin P1126), PDB AF_AFA0A023IKK2F1 (MHC Class II Beta Chain) and PDB AF_AFA0A023GPK8F1 (Friend of Echinoid, Isoform H). These were obtained from the Computed Structure Models (CSM) section of the RCSB PDB42. Visualisations of biomolecular structures were created using ChimeraX29,69,83,84. All other figure elements (including biomolecular structures at atomic resolution, electronic densities, absorption spectra and atomic energies) were generated with Matplotlib74 for python. References
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Metadata
- Authors
- Garcia, M., & Wieners, L.
- Affiliations
- Universität Kassel
- University of Kassel (DE)
- Venue
- Communications Chemistry
- Published
- 2025-09-16
- Volume
- 9
- Issue
- 1
- ISSN
- 2399-3669 (ISSN-L)
- PMC
- PMC12458572
- OpenAlex
- W7159083704
- Cited by
- 1
- References
- 2
- Citations by year
- 2026: 1
- FWCI
- 2.56
- Type
- journal article
- Language
- en
- Open access
- gold
- doi.org
- Locations
- Communications Chemistry (publishedVersion, cc-by)
- Research Square (acceptedVersion, cc-by)
- PubMed (publishedVersion)
- PubMed Central (publishedVersion, cc-by)
- Europe PMC (PubMed Central) (submittedVersion, cc-by)
- DOAJ (DOAJ: Directory of Open Access Journals) (submittedVersion, cc-by-sa)
- Kobra (Universitätsbibliothek Kassel) (cc-by)
- Funders
- Deutsche Forschungsgemeinschaft (RTG 2749/1, RTG 2749, GRK2749-1)
- Technische Universität Darmstadt
- Universität Kassel
- National Institutes of Health
- University of California, San Francisco (R01-GM129325)
- National Institute of General Medical Sciences (R01GM129325)
- National Institute of Allergy and Infectious Diseases
- Topics
- Physical Sciences › Physics and Astronomy › Atomic and Molecular Physics, and Optics › Advanced Chemical Physics Studies
- Physical Sciences › Chemistry › Physical and Theoretical Chemistry › Advanced Physical and Chemical Molecular Interactions
- Life Sciences › Biochemistry, Genetics and Molecular Biology › Molecular Biology › Protein Structure and Dynamics
- Keywords
- divide-and-conquer, minimal basis sets, computational efficiency
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- The paper
- Garcia, M., & Wieners, L. (2025). Bridging Quantum Mechanics and Biology at the Million-Atom Scale. Communications Chemistry. https://doi.org/10.21203/rs.3.rs-7327472/v1