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Spin Space Symmetry Without Spin Space Groups

Strongly Correlated Electrons · Submitted 27 Oct 2026

abstract compiled · 2026-10-30 · no language-model review

The authors' main claim We argue that working directly with this representation not only avoids the construction and identification of the group, but also organizes and simplifies the resulting symmetry constraints on allowed responses.

how it is stated · asserted 0.87 read the record →

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arXiv ID2610.37770 (version 1)
Pith ID7SSYRMBH, Pith's permanent record of this paper and its review
CitationJeffrey G. Rau. "Spin Space Symmetry Without Spin Space Groups." arXiv:2610.37770 (2026). https://pith.science/paper/7SSYRMBH
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Compiled by classifier-1.13.0 via TypeSafe API, question bank abstract-p1-20260923, 2026-10-30: 1 request, 8,315 input tokens.

What the abstract itself states, as probabilities: claims first 0.04 · states limitation 0.30 · human participants 0.01 · controlled comparison 0.02 · randomized assignment 0.01 · states quantitative result 0.09 · compares with prior results 0.59 · mentions code or data availability 0.02.

The abstract, sentence by sentence

arXiv listing abstract v1. Results and the main claim are underlined; .

Spin space groups provide a complete symmetry classification of magnetic structures in the non-relativistic limit and have become an increasingly useful language for organizing magnetic phases and their physical properties. Each spin space group with a given parent space group is specified, up to spin-only symmetries, by a real representation of that space group acting in spin space. We argue that working directly with this representation not only avoids the construction and identification of the group, but also organizes and simplifies the resulting symmetry constraints on allowed responses. Determining the presence or absence of magnetic compensation, piezomagnetism, spin and charge transport, the Edelstein effect, and momentum-space spin textures becomes an ordinary problem in the representation theory of space groups. The resulting conditions reduce to overlaps between the three exterior powers of the defining representation and multipole representations of the point group. Several physically distinct responses then reduce to the same condition on the defining representation. For example, a $p$-wave spin texture and the time-even Edelstein effect are allowed under the same condition, as are piezomagnetism and a $d$-wave spin texture in compensated order. The wave-vector content of the exterior powers gives a further hierarchy of selection rules: depending on the relevant power, a uniform response requires one, two, or three ordering wave vectors to sum to a reciprocal lattice vector. These rules can exclude many responses before point-group symmetry is considered. We illustrate the approach with examples drawn from a wide variety of materials hosting collinear, coplanar and non-coplanar magnetic order. Finally, we discuss extensions of these results to magnetic space groups, connections to Landau theories of collinear order, and the characterization of odd-parity magnets.

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What the classifier reports for each sentence. The number is the probability it gave the label.
#sentencerolethe authors' own workstates the main conclusionstrength
s0 Spin space groups provide a complete symmetry classification of magnetic structures in the non-relativistic limit and have become an increasingly useful language for organizing magnetic phases and their physical properties. background 1.00 0.05 0.05 asserted 1.00
s1 Each spin space group with a given parent space group is specified, up to spin-only symmetries, by a real representation of that space group acting in spin space. background 0.97 0.10 0.06 asserted 1.00
s2 We argue that working directly with this representation not only avoids the construction and identification of the group, but also organizes and simplifies the resulting symmetry constraints on allowed responses. contribution 0.69 0.47 0.49 asserted 0.87
s3 Determining the presence or absence of magnetic compensation, piezomagnetism, spin and charge transport, the Edelstein effect, and momentum-space spin textures becomes an ordinary problem in the representation theory of space groups. result 0.41 0.58 0.27 asserted 1.00
s4 The resulting conditions reduce to overlaps between the three exterior powers of the defining representation and multipole representations of the point group. result 0.73 0.83 0.17 asserted 1.00
s5 Several physically distinct responses then reduce to the same condition on the defining representation. result 0.80 0.77 0.15 asserted 0.99
s6 For example, a $p$-wave spin texture and the time-even Edelstein effect are allowed under the same condition, as are piezomagnetism and a $d$-wave spin texture in compensated order. result 0.88 0.78 0.10 asserted 0.96
s7 The wave-vector content of the exterior powers gives a further hierarchy of selection rules: depending on the relevant power, a uniform response requires one, two, or three ordering wave vectors to sum to a reciprocal lattice vector. result 0.87 0.80 0.07 asserted 0.99
s8 These rules can exclude many responses before point-group symmetry is considered. result 0.55 0.69 0.06 hedged possibility 0.57
s9 We illustrate the approach with examples drawn from a wide variety of materials hosting collinear, coplanar and non-coplanar magnetic order. contribution 0.57 0.86 0.04 asserted 0.99
s10 Finally, we discuss extensions of these results to magnetic space groups, connections to Landau theories of collinear order, and the characterization of odd-parity magnets. future work 0.94 0.75 0.06 asserted 0.68

What kind of paper the classifier reports this is: method or tool 0.82 · evidence from proof or derivation 0.80.

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Every quoted sentence on this record is the authors'. Every label is from Pith's closed vocabulary, with the probability shown beside it. Every number in the measurements table is the authors', checked by code. Record as JSON

The paper
Original abstract

Spin space groups provide a complete symmetry classification of magnetic structures in the non-relativistic limit and have become an increasingly useful language for organizing magnetic phases and their physical properties. Each spin space group with a given parent space group is specified, up to spin-only symmetries, by a real representation of that space group acting in spin space. We argue that working directly with this representation not only avoids the construction and identification of the group, but also organizes and simplifies the resulting symmetry constraints on allowed responses. Determining the presence or absence of magnetic compensation, piezomagnetism, spin and charge transport, the Edelstein effect, and momentum-space spin textures becomes an ordinary problem in the representation theory of space groups. The resulting conditions reduce to overlaps between the three exterior powers of the defining representation and multipole representations of the point group. Several physically distinct responses then reduce to the same condition on the defining representation. For example, a $p$-wave spin texture and the time-even Edelstein effect are allowed under the same condition, as are piezomagnetism and a $d$-wave spin texture in compensated order. The wave-vector content of the exterior powers gives a further hierarchy of selection rules: depending on the relevant power, a uniform response requires one, two, or three ordering wave vectors to sum to a reciprocal lattice vector. These rules can exclude many responses before point-group symmetry is considered. We illustrate the approach with examples drawn from a wide variety of materials hosting collinear, coplanar and non-coplanar magnetic order. Finally, we discuss extensions of these results to magnetic space groups, connections to Landau theories of collinear order, and the characterization of odd-parity magnets.

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