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arxiv: 2605.12907 · v1 · submitted 2026-05-13 · ❄️ cond-mat.str-el

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Grassmann tensor networks

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The pith

Grassmann tensor networks are introduced from basic operations to algorithm Grassmannization and validated on models from particle physics and condensed matter.

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

Fermions like electrons follow special rules where swapping two particles changes the sign of the wavefunction. Tensor networks represent large quantum systems by connecting small tensors in a network to avoid exponential cost. Grassmann algebra supplies anticommuting numbers that match fermion statistics in path integrals. The paper walks through how to perform tensor operations with these Grassmann numbers and converts common tensor-network algorithms such as renormalization or contraction into their Grassmann versions. It then tests the resulting methods on example models from both condensed-matter and particle-physics settings.

Core claim

Grassmann tensor network methods offer powerful numerical tools for fermionic many-body systems in the coherent-state path-integral representation and are validated in several interesting models in both particle physics and condensed matter physics.

Load-bearing premise

That the Grassmann tensor operations and their Grassmannized algorithms can be implemented efficiently enough for practical simulations of strongly correlated systems without prohibitive computational overhead or sign problems.

Figures

Figures reproduced from arXiv: 2605.12907 by Jia-Ji Zhu, Jian-Gang Kong, Z. Y. Xie.

Figure 1
Figure 1. Figure 1: Decompose a rank-4 Grassmann tensor T to two rank-3 Grassmann tensors A and B by singular value decomposition, as expressed in Eqs. (43-44). Note, in Eqs. (41-42), the Λ is a positive definite diagonal matrix with no Grassmann counterpart defined, U˜ is a column-wise orthogonal matrix, and V˜ is row-wise orthog￾onal. Once Eq. (41) is obtained, then we can absorb the ordinary matrix Λ into U and V to obtain… view at source ↗
Figure 2
Figure 2. Figure 2: An effective (1+1)-dimensional lattice with coordinates [PITH_FULL_IMAGE:figures/full_fig_p025_2.png] view at source ↗
Figure 3
Figure 3. Figure 3: (a) The decomposition of the Grassmann exponents, as expressed in Eq. ( [PITH_FULL_IMAGE:figures/full_fig_p029_3.png] view at source ↗
Figure 4
Figure 4. Figure 4: The Grassmann generalization of the (a) left-canonical condition and (b) right-canonical   [PITH_FULL_IMAGE:figures/full_fig_p038_4.png] view at source ↗
Figure 5
Figure 5. Figure 5: Ground-state properties of the half-filled Hubbard model given by Eq. ( [PITH_FULL_IMAGE:figures/full_fig_p040_5.png] view at source ↗
Figure 6
Figure 6. Figure 6: Free energy density f versus inverse temperature β for the one-dimensional free-fermion model at µ = 2.0, obtained via the Grassmann TEBD algorithm in the coherent-state path-integral formalism. Curves correspond to different temporal steps ϵ and bond dimensions χ. The black line indicates the exact analytic result [PITH_FULL_IMAGE:figures/full_fig_p046_6.png] view at source ↗
Figure 7
Figure 7. Figure 7: Relative error δf of the free energy density for the single-flavor, non-interacting GNW model at m = −1.2, comparing Grassmann CTMRG, Grassmann TEBD, and Grassmann TRG methods at various bond dimensions χ [PITH_FULL_IMAGE:figures/full_fig_p053_7.png] view at source ↗
Figure 8
Figure 8. Figure 8: Applying the Grassmann gate G (α) to bond α in the Grassmann SU algorithm involves the following steps: (i) preprocessing, (ii) contraction and truncation and (iii) renormalization, leading to updated local tensors A, B and Λα. as Amk1k2k3 = Amk1k2k3ψ¯p(m) m ¯ξ p(k1) 1 ¯ξ p(k2) 2 ¯ξ p(k3) 3 , (227) Bnk1l2l3 = Bnk1l2l3ψ¯p(n) n ξ p(k1) 1 ξ p(l2) 2 ξ p(l3) 3 , (228) G (α) ijmn = G (α) ijmnφ¯ p(i) i φ¯ p(j) j … view at source ↗
Figure 9
Figure 9. Figure 9: Energy per link for the free-fermion model in Eq. ( [PITH_FULL_IMAGE:figures/full_fig_p061_9.png] view at source ↗
Figure 10
Figure 10. Figure 10: For the t-V1-V2 model at V1 = −1.0 and V2 = 0.5: (a) Convergence of the particle density n with Grassmann CTMRG environment dimension χ at µ = 0. (b) Energy per site Es versus particle density n. Red cross denotes data from the large-scale (non-Grassmann) DMRG calculation. At µ = 0.0, the particle-hole symmetry of the Hamiltonian dictates an exact av￾erage density of n = 0.5. This is confirmed numerically… view at source ↗
read the original abstract

Developing non-perturbative methods to reveal exotic properties of strongly correlated fermionic systems remains one of the most essential tasks of theoretical physics. Tensor network methods with Grassmann algebra offer powerful numerical tools for fermionic many-body systems in the coherent-state path-integral representation. Despite their vast potential for both condensed-matter and particle-physics communities, Grassmann tensor network methods are somewhat underexploited in practical simulations. In this work, we provide a detailed, self-contained introduction to Grassmann tensor network methods, from the basics of the Grassmann tensor operations to the Grassmannization of typical tensor network algorithms. Furthermore, the resulting Grassmann tensor network methods are validated in several interesting models in both particle physics and condensed matter physics.

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

0 major / 2 minor

Summary. The manuscript provides a detailed, self-contained introduction to Grassmann tensor network methods for fermionic many-body systems in the coherent-state path-integral representation. It covers the fundamentals of Grassmann tensor operations, the Grassmannization of standard tensor network algorithms, and reports validations of the resulting methods on several models drawn from both particle physics and condensed matter physics.

Significance. If the validations hold under scrutiny, the work has clear value in lowering the barrier to practical use of Grassmann tensor networks for strongly correlated fermions, a class of methods that the abstract correctly notes remains underexploited. The self-contained derivation of the operations and algorithms is a concrete strength that could facilitate adoption across communities.

minor comments (2)
  1. [Abstract] The abstract states that validations were performed on several models but does not name the models or the key observables; adding one sentence would improve the reader's immediate grasp of the scope without lengthening the abstract.
  2. [Basics of Grassmann tensor operations] In the sections introducing Grassmann tensor operations, the distinction between the Grassmann parity and the tensor indices could be illustrated with a small explicit example to aid readers unfamiliar with the algebra.

Simulated Author's Rebuttal

0 responses · 0 unresolved

We thank the referee for the positive assessment and recommendation for minor revision. The report correctly identifies the manuscript's self-contained introduction to Grassmann tensor operations and algorithms, along with validations across particle-physics and condensed-matter models. No specific major comments were raised that require point-by-point rebuttal.

Circularity Check

0 steps flagged

No significant circularity in derivation chain

full rationale

The paper frames itself as a self-contained introduction to Grassmann tensor operations and algorithms, starting from standard Grassmann algebra basics and proceeding to Grassmannized tensor network methods without any load-bearing steps that reduce by construction to fitted parameters, self-definitions, or self-citation chains. Validations on models are presented as applications of the derived methods rather than circular predictions. No equations or claims in the abstract or described structure exhibit the enumerated circularity patterns.

Axiom & Free-Parameter Ledger

0 free parameters · 1 axioms · 0 invented entities

The central claim rests on standard mathematical properties of Grassmann algebra and tensor-network contraction rules already present in the prior literature; no new free parameters, ad-hoc axioms, or postulated entities are introduced in the abstract.

axioms (1)
  • standard math Grassmann algebra supplies anticommuting variables that correctly encode fermionic statistics in coherent-state path integrals
    Invoked as the foundation for the entire representation of fermionic systems.

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