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BF Couplings and Discrete Topological Data

A compact BF coupling pairs two higher-form gauge connections of complementary degree. Its local equations set their curvatures to zero, while the sum over compact global sectors retains finite holonomy. At integer level NN, the resulting electric and magnetic operators carry labels in ZN\mathbb Z_N, and linked complementary supports acquire an NNth-root-of-unity phase. That conclusion uses compactness, the integral flux lattice, and the global path-integral sum; it does not follow from the local density BdAB\wedge\mathrm dA alone.

This page starts on a closed smooth oriented DD-manifold and uses the Euclidean weight eSEe^{-S_E}. It then opens a boundary and threads the same global-definition test through four-dimensional Higgs theory, three-dimensional Abelian Chern–Simons theory, compact BF theory, and finite gauge theory. Fixed fields define a response phase; integrating the same fields defines a dynamical theory and is a logically separate choice.

Required background. When Is a Topological Term Well Defined? supplies the exponentiated-action and period tests used to quantize the BF coefficient. Differential Forms, Integration, and Stokes’ Theorem supplies the degree counting, orientation, and boundary formula.

Helpful background. Gauging a Higher-Form Symmetry separates a local coupling from the global sum over gauge fields. Linking, Braiding, and Framing fixes the complementary-support linking convention. Chains, Homology, Cohomology, and Exact Sequences supplies the finite-coefficient and torsion information that ordinary differential forms miss.

Compact BF theory pairs two higher-form connections

Section titled “Compact BF theory pairs two higher-form connections”

Let MDM^D be closed, smooth, and oriented, and choose 1pD21\leq p\leq D-2. Let ApA_p be a compact U(1)U(1) pp-form connection and BDp1B_{D-p-1} a compact U(1)U(1) (Dp1)(D-p-1)-form connection. Their curvatures have 2π2\pi-integral periods. In a simultaneous local trivialization, the Euclidean BF action is

SEloc[A,B]=iN2πMBDp1dAp,NZ.S_E^{\mathrm{loc}}[A,B] = \frac{iN}{2\pi} \int_M B_{D-p-1}\wedge\mathrm dA_p, \qquad N\in\mathbb Z.

The degrees add correctly:

degB+(degA+1)=(Dp1)+(p+1)=D.\deg B+(\deg A+1)=(D-p-1)+(p+1)=D.

For the finite theory below take N1N\geq1; the sign of a nonzero NN can be reversed by BBB\mapsto-B. Locally the gauge transformations are

AA+dαp1,BB+dβDp2.A\longmapsto A+\mathrm d\alpha_{p-1}, \qquad B\longmapsto B+\mathrm d\beta_{D-p-2}.

Large transformations and nontrivial bundles are not exhausted by these exact shifts. A compact higher connection is described by compatible patch, overlap, and integral cocycle data. Intrinsically one may package the fields as differential cohomology classes

AˇH^p+1(M;Z),BˇH^Dp(M;Z),\check A\in\widehat H^{p+1}(M;\mathbb Z), \qquad \check B\in\widehat H^{D-p}(M;\mathbb Z),

and define the phase through their differential-cohomology product. With the ordering chosen to reproduce BdAB\wedge\mathrm dA locally,

eSE[A,B]=exp ⁣[2πiNMBˇAˇ].e^{-S_E[A,B]} = \exp\!\left[ -2\pi iN\int_M\check B\smile\check A \right].

The integral here is valued in R/Z\mathbb R/\mathbb Z. It retains flat and torsion data even when every de Rham curvature vanishes. The ordinary form integral is therefore useful local shorthand, not the complete global definition. Kapustin and Seiberg give an explicit compact-field construction and its Deligne–Beilinson completion in Kapustin and Seiberg 2014, § 3, arXiv v2, printed pp. 9–12, eqs. (3.1)–(3.13), PDF.

No metric appears in the BF phase. That establishes metric independence of this term, not by itself a complete topological quantum field theory. The field role still matters:

  • if AA and BB are fixed backgrounds, the phase is an invertible response;
  • if one field is summed, it imposes a compact Fourier constraint on the other; and
  • if both are summed, the result is a dynamical compact BF theory.

Integer level turns flatness into finite holonomy

Section titled “Integer level turns flatness into finite holonomy”

The coefficient lattice follows from the exponentiated action. Let BB+2πβB\mapsto B+2\pi\beta, where β\beta is a closed integral (Dp1)(D-p-1)-form, and let dA/(2π)\mathrm dA/(2\pi) represent an integral curvature class. Then

ΔSE=iN2πM2πβdA=2πiNMβdA2π.\Delta S_E = \frac{iN}{2\pi} \int_M 2\pi\beta\wedge\mathrm dA = 2\pi iN \int_M\beta\wedge\frac{\mathrm dA}{2\pi}.

The last integral is an integer. Hence eSEe^{-S_E} is invariant for NZN\in\mathbb Z. When the allowed compact sectors realize a unit pairing, integrality is also necessary. A restricted charge or flux lattice can change the allowed coefficient lattice, so the bare assertion “NN is an integer” always includes the standard compact normalization used here. The large-gauge calculation is made explicit in Kapustin and Seiberg 2014, § 3, arXiv v2, printed p. 11, eq. (3.6), PDF.

Varying the local action on a closed manifold gives, away from operator insertions,

dA=0,dB=0.\mathrm dA=0, \qquad \mathrm dB=0.

These are curvature equations. They do not imply that either compact connection is gauge-equivalent to zero. A flat connection can have nontrivial holonomy around a noncontractible cycle, including torsion holonomy invisible to a real differential form.

The compact path integral sharpens the statement. Summing one field performs a finite Fourier projection, so the surviving holonomies obey

N2πAZ,N2πBZ\frac{N}{2\pi}\oint A\in\mathbb Z, \qquad \frac{N}{2\pi}\oint B\in\mathbb Z

on the corresponding cycles. Thus their values are NNth roots of unity, and the finite labels lie in ZN\mathbb Z_N. Gauge-equivalence classes of a flat pp-form ZN\mathbb Z_N connection are organized by

Hp(M;ZN).H^p(M;\mathbb Z_N).

Brennan and Hong derive the Fourier projection, the finite holonomy, and the operator labels from the compact BF sum in Brennan and Hong 2023, § 3, arXiv v2, printed pp. 32–34, eqs. (3.22)–(3.35), PDF. Replacing either compact field by an unconstrained real form destroys the integral sector sum and does not produce a ZN\mathbb Z_N gauge theory.

Linked Wilson operators measure the mixed pairing

Section titled “Linked Wilson operators measure the mixed pairing”

Let CpC_p and ΣDp1\Sigma_{D-p-1} be disjoint closed oriented supports. Their dimensions add to D1D-1, so they can link in DD dimensions. For the ordinary integer linking number below, assume that Σ\Sigma bounds over the relevant coefficients, equivalently that a global ηΣ\eta_\Sigma can be chosen; this is automatic for the local examples on a sphere. If the correlator is written as a ratio, also work in a sector where the two one-point normalizations are nonzero. General manifolds instead require the torsion or differential-cohomology pairing developed in the next section. Define

We(C):=exp ⁣(ieCA),Vm(Σ):=exp ⁣(imΣB),W_e(C) := \exp\!\left(ie\int_C A\right), \qquad V_m(\Sigma) := \exp\!\left(im\int_\Sigma B\right),

with e,mZe,m\in\mathbb Z. Fix the orientation convention by choosing a form ηΣ\eta_\Sigma with dηΣ=δΣ\mathrm d\eta_\Sigma=\delta_\Sigma and setting

Lk(C,Σ):=CηΣ.\operatorname{Lk}(C,\Sigma) := \int_C\eta_\Sigma.

In the Euclidean convention of this page, integrating over BB in the presence of Vm(Σ)V_m(\Sigma) fixes the sourced curvature of AA. Substitution into We(C)W_e(C) gives the mixed topological factor

We(C)Vm(Σ)We(C)Vm(Σ)=exp ⁣[2πiemNLk(C,Σ)].\frac{\left\langle W_e(C)V_m(\Sigma)\right\rangle} {\left\langle W_e(C)\right\rangle \left\langle V_m(\Sigma)\right\rangle} = \exp\!\left[ \frac{2\pi i\,em}{N} \operatorname{Lk}(C,\Sigma) \right].

The sign is fixed by the displayed eSEe^{-S_E} convention and the definition of linking above. Reversing the orientation of either support changes the linking number’s sign and complex-conjugates the phase. The charges are defined modulo NN: shifting ee or mm by NN leaves every mixed phase unchanged. At N=1N=1 the finite linking data are trivial.

In four dimensions with p=1p=1, WeW_e is a line and VmV_m is a surface. In three dimensions with p=1p=1, both supports are lines. The same formula then becomes mutual line braiding. The compact normalization and positive linking phase agree with Banks and Seiberg 2011, § 2, arXiv v2, printed p. 8, eqs. (2.12)–(2.13), PDF and Brennan and Hong 2023, § 3, arXiv v2, printed pp. 33–34, eqs. (3.29)–(3.35), PDF.

The finite cohomology group above contains more than reductions of smooth de Rham periods. The universal-coefficient sequence gives

0ExtZ1 ⁣(Hp1(M;Z),ZN)Hp(M;ZN)HomZ ⁣(Hp(M;Z),ZN)0.0\longrightarrow \operatorname{Ext}_{\mathbb Z}^{1} \!\left(H_{p-1}(M;\mathbb Z),\mathbb Z_N\right) \longrightarrow H^p(M;\mathbb Z_N) \longrightarrow \operatorname{Hom}_{\mathbb Z} \!\left(H_p(M;\mathbb Z),\mathbb Z_N\right) \longrightarrow0.

The sequence splits noncanonically. Its left term records finite-coefficient classes not visible from homomorphisms on pp-cycles alone. If Hp(M)H_p(M) contains a cyclic direct summand Z\mathbb Z_\ell, then that summand contributes

Hom(Z,ZN)Zgcd(,N).\operatorname{Hom}(\mathbb Z_\ell,\mathbb Z_N) \cong \mathbb Z_{\gcd(\ell,N)}.

Thus a cyclic direct summand of order \ell contributes gcd(,N)\gcd(\ell,N) compatible finite holonomies—not automatically \ell and not automatically NN. For an order-\ell cycle embedded in a larger homology group, the available values form the image of the restriction map to its cyclic subgroup and can be smaller. Equivalently, if γ=Γ\ell\gamma=\partial\Gamma, a globally defined torsion operator must combine the integral over Γ\Gamma with holonomy data on γ\gamma; the local form integral over Γ\Gamma alone is not gauge invariant. Kapustin and Seiberg construct this operator and show that its order divides gcd(N,)\gcd(N,\ell) in Kapustin and Seiberg 2014, § 3, arXiv v2, printed p. 12, eqs. (3.11)–(3.13), PDF.

This is the precise sense in which BF theory can be locally flat and globally nontrivial. Curvature probes the free real part of cohomology; compact cocycles, holonomies, and linking pairings retain the finite part.

First application: a charge-N Higgs phase becomes compact BF theory

Section titled “First application: a charge-N Higgs phase becomes compact BF theory”

Take a four-dimensional Euclidean theory on a closed oriented manifold X4X^4 with a compact U(1)U(1) connection AA, normalized by

12πΣ2dAZ.\frac{1}{2\pi}\int_{\Sigma_2}\mathrm dA\in\mathbb Z.

Let a charge-NN scalar condense while no lower-charge field condenses. At fixed radial mode write

Φ=veiφ,φφ+2π,φφ+Nλ,AA+dλ.\Phi=v e^{i\varphi}, \qquad \varphi\sim\varphi+2\pi, \qquad \varphi\longmapsto\varphi+N\lambda, \qquad A\longmapsto A+\mathrm d\lambda.

The phase stiffness contains

Sphase=v22X4(dφNA)(dφNA).S_{\mathrm{phase}} = \frac{v^2}{2} \int_{X^4} (\mathrm d\varphi-NA)\wedge *\,(\mathrm d\varphi-NA).

Dualizing the periodic scalar gives a compact two-form connection BB. Up to metric-dependent kinetic terms, the dual Euclidean action contains

SEdual=Skin[A,B]+iN2πX4BdA.S_E^{\mathrm{dual}} = S_{\mathrm{kin}}[A,B] + \frac{iN}{2\pi} \int_{X^4}B\wedge\mathrm dA.

The kinetic terms are suppressed deep in the gapped infrared, leaving the compact BF phase. Periodicity of φ\varphi is what makes BB compact; the local dualization without the winding-sector sum would not recover the finite global theory. The charge-NN Higgs derivation and its normalization are worked out in Banks and Seiberg 2011, § 2, arXiv v2, printed pp. 6–8, eqs. (2.3)–(2.13), PDF and Brennan and Hong 2023, § 3, arXiv v2, printed pp. 35–36, eqs. (3.36)–(3.45), PDF.

The surviving operators are the Wilson line Wq(C)W_q(C) and the vortex surface Vm(Σ)V_m(\Sigma). For a once-linked unit pair at N=3N=3,

Lk(C,Σ)=1W1(C)V1(Σ)W1(C)V1(Σ)=e2πi/3.\operatorname{Lk}(C,\Sigma)=1 \quad\Longrightarrow\quad \frac{\langle W_1(C)V_1(\Sigma)\rangle} {\langle W_1(C)\rangle\langle V_1(\Sigma)\rangle} =e^{2\pi i/3}.

Reversing either support gives e2πi/3e^{-2\pi i/3}, and three units of either charge have trivial mutual phase. This is a direct infrared measurement of the residual Z3\mathbb Z_3 data.

The threaded comparison keeps field role and global data visible

Section titled “The threaded comparison keeps field role and global data visible”

The four rows below apply the same questions—what is global, what is summed, and what is quantized—without identifying theories of different dimension or different field content. The Chern–Simons and finite-gauge rows are bounded comparators, not derivations from the four-dimensional Higgs model.

One global-definition test across the threaded Abelian Chern–Simons, compact BF, and finite-gauge comparison; the rows are not equivalent theories
Model and field role Global datum Quantized input Operator check What does not follow
4d compact BF from the Higgs phase; both fields dynamical Compact one- and two-form connections, including torsion sectors Integer charge and BF level N Line–surface phase is an Nth root of unity The local flatness equations alone do not reconstruct the compact sector sum
3d compact Abelian BF; both one-form fields dynamical An integral off-diagonal K-matrix and compact bundles K has off-diagonal entries N Mutual line phase is an Nth root of unity Twists and boundary data are not fixed by the untwisted BF coefficient
3d Abelian Chern–Simons; background or dynamical connection declared separately A differential characteristic class and its spin or oriented refinement The allowed level lattice, not a theta-period identification Line–line braiding and self-linking require framing data A quantized local coefficient does not decide invertibility or the field role
Finite Dijkgraaf–Witten gauge theory; finite bundles summed A finite gauge group, flat bundles, measure, and cocycle class A discrete cohomology class rather than a continuous BF level Bundle holonomies and cocycle-weighted amplitudes A generic finite gauge theory need not admit this Abelian BF presentation

One bounded state-space check makes the finite sector count concrete. In an untwisted AA-polarization on a closed spatial manifold YY, a basis is labeled by the finite flat sectors,

dimH(Y)=Hp(Y;ZN).\dim\mathcal H(Y) = \left\lvert H^p(Y;\mathbb Z_N)\right\rvert.

Consequently the three-dimensional p=1p=1 theory has dimH(T2)=N2\dim\mathcal H(T^2)=N^2, while the four-dimensional p=1p=1 theory has dimH(T3)=N3\dim\mathcal H(T^3)=N^3. The conjugate BB holonomies act as finite clock and shift operators on this space; they are not a second independent set of basis labels to be multiplied in again. On a lens space Y=L(,q)Y=L(\ell,q), the same formula gives dimH(Y)=gcd(N,)\dim\mathcal H(Y)=\gcd(N,\ell), matching the torsion calculation above. The flat-bundle state construction appears in Dijkgraaf and Witten 1990, § 6.3, printed pp. 416–417, eqs. (6.15)–(6.17); the canonical four-dimensional BF count is given in Bergeron, Semenoff, and Szabo 1995, § 4.1, arXiv v1, printed p. 18, PDF.

In three dimensions, untwisted compact BF theory can be written in the Abelian KK-matrix form

KBF=(0NN0),detKBF=N2.K_{\mathrm{BF}} = \begin{pmatrix} 0&N\\ N&0 \end{pmatrix}, \qquad \det K_{\mathrm{BF}}=-N^2.

The genus-gg Abelian Chern–Simons state-space count is detKg\lvert\det K\rvert^g, so on a two-torus

dimH(T2)=N2.\dim\mathcal H(T^2)=N^2.

For N>1N>1 this immediately rules out invertibility of the dynamical theory. Belov and Moore give the determinant count in Belov and Moore 2005, § 5.3, printed p. 26, immediately after eq. (5.17), PDF. A bosonic Abelian twist may be encoded by

Kr=(2rNN0),rZN.K_r = \begin{pmatrix} 2r&N\\ N&0 \end{pmatrix}, \qquad r\in\mathbb Z_N.

Its determinant remains N2-N^2, but its spins and braiding data change. In the compact-field convention of Kapustin and Seiberg, their diagonal coefficient is pKS=2rp_{\mathrm{KS}}=2r for an ordinary oriented bosonic Dijkgraaf–Witten class; odd pKSp_{\mathrm{KS}} instead requires spin data. Thus NN fixes the untwisted mixed pairing but does not classify every finite topological term. The continuum action and coefficient identification are given in Kapustin and Seiberg 2014, § 5, arXiv v2, printed pp. 20–21, eqs. (5.1)–(5.3), PDF.

For r=0r=0, compact three-dimensional BF theory realizes the untwisted ZN\mathbb Z_N finite gauge theory after the global sector sum and measure are matched. This is a statement about the completed quantum theory, not an identity inferred from a local Euler–Lagrange equation. Dijkgraaf and Witten construct the finite-bundle sum and cocycle weights in Dijkgraaf and Witten 1990, § 6.2, printed pp. 415–416, eqs. (6.8)–(6.10).

Now let MM have a boundary. Under the local BB-field gauge transformation BB+dΛB\mapsto B+\mathrm d\Lambda,

ΔΛSE=iN2πMdΛdA=iN2πMΛdA,\Delta_\Lambda S_E = \frac{iN}{2\pi} \int_M\mathrm d\Lambda\wedge\mathrm dA = \frac{iN}{2\pi} \int_{\partial M}\Lambda\wedge\mathrm dA,

where the final sign uses the induced boundary orientation. By contrast, AA+dαA\mapsto A+\mathrm d\alpha leaves the displayed local curvature dA\mathrm dA unchanged. Global gauge invariance still belongs to the full differential-cocycle definition.

There is a second, independent boundary issue. An arbitrary variation of AA produces a boundary term proportional to

MBδA,\int_{\partial M}B\wedge\delta A,

with the sign fixed by DD and pp. A well-posed theory therefore needs a choice such as fixed boundary pullback of AA, a complementary polarization, restricted boundary gauge transformations, a boundary counterterm that swaps the polarization, or additional boundary fields whose variation cancels the bulk term. The local BF density selects none of these choices by itself. Kapustin and Seiberg display one concrete completion in Kapustin and Seiberg 2014, § 6, arXiv v2, printed pp. 25–26, eqs. (6.19)–(6.25), PDF; it is an example, not a universal boundary theory.

What the BF coupling establishes—and what it leaves open

Section titled “What the BF coupling establishes—and what it leaves open”

The compact BF term establishes a robust set of statements within the declared normalization:

  • the integer level is required by large compact gauge transformations;
  • the local equations impose curvature flatness;
  • the compact global sum reduces continuous holonomy to finite ZN\mathbb Z_N data;
  • complementary Wilson supports measure the mixed linking pairing; and
  • torsion sectors require global cocycles rather than de Rham forms alone.

It does not, by itself, determine every datum of the completed theory. A finite cocycle twist, a spin refinement, a boundary polarization, kinetic deformations away from the infrared, the path-integral normalization, and the full state-space and gluing assignments are additional inputs. Nor does coefficient quantization imply invertibility: the fixed-field BF response is invertible as a phase, while the dynamical N>1N>1 BF theory has multi-dimensional state spaces.

The next BF Theory as a Topological Gauge Theory treatment will develop the state spaces, gluing maps, observables, and exact topological data. Finite Gauge Theory and Dijkgraaf–Witten Twists will separate untwisted BF presentations from general cocycle-twisted finite gauge theories. The already developed Chern–Simons Actions and Level Quantization treatment supplies the self-pairing, spin, boundary, and framing side of the comparison.

Flat does not mean trivial. The equations dA=dB=0\mathrm dA=\mathrm dB=0 remove local curvature. They leave holonomy and torsion sectors, which are precisely where the finite gauge data live.

A noncompact BF density does not define a finite gauge theory. The ZN\mathbb Z_N conclusion uses compact higher connections, integral fluxes, and the sum over global sectors. Dropping those ingredients changes the theory even though the local Euler–Lagrange equations look the same.

An integer coefficient does not make a dynamical theory invertible. A fixed BF phase has a stacking inverse, but the dynamical three-dimensional N>1N>1 theory already has N2N^2 states on T2T^2.

Boundary variation does not select a unique edge theory. It identifies data that must be completed. Boundary conditions, polarizations, counterterms, and boundary fields are distinct completions with different physics.

Untwisted BF is not every finite gauge theory. In the cyclic Abelian KK-matrix family above, a cocycle twist changes spins and braiding while detK=N2\lvert\det K\rvert=N^2 and the torus-state count stays fixed. Twists for a generic finite group need not preserve that count, and non-Abelian theories require data not captured by the displayed Abelian form.

1. Degree check. In D=7D=7, let AA be a two-form connection. What is the degree of BB, and what dimensions do the two complementary Wilson supports have?

Solution

Here p=2p=2, so BB has degree Dp1=4D-p-1=4. The AA operator is supported on a two-cycle and the BB operator on a four-cycle. Their dimensions add to six, which is D1D-1, so disjoint supports can link in seven dimensions.

2. Large-gauge check. Suppose MβdA/(2π)=3\int_M\beta\wedge\mathrm dA/(2\pi)=3. What happens to the Euclidean weight under BB+2πβB\mapsto B+2\pi\beta?

Solution

The action changes by ΔSE=6πiN\Delta S_E=6\pi iN. Therefore eSEeSEe6πiN=eSEe^{-S_E}\mapsto e^{-S_E}e^{-6\pi iN}=e^{-S_E} for integer NN.

3. Linking check. For N=5N=5, e=2e=2, m=3m=3, and Lk(C,Σ)=1\operatorname{Lk}(C,\Sigma)=-1, compute the mixed phase.

Solution

The phase is exp[12πi/5]=exp[2πi/5]\exp[-12\pi i/5]=\exp[-2\pi i/5]. Reducing the charges modulo five gives the same result. Reversing either support changes it to exp[2πi/5]\exp[2\pi i/5].

4. Torsion check. Suppose Hp(M)H_p(M) has a cyclic direct summand Z12\mathbb Z_{12} generated by γ\gamma. How many Z8\mathbb Z_8 holonomies can this summand support?

Solution

Hom(Z12,Z8)\operatorname{Hom}(\mathbb Z_{12},\mathbb Z_8) is Zgcd(12,8)=Z4\mathbb Z_{\gcd(12,8)}=\mathbb Z_4. There are four compatible holonomies. Ordinary de Rham periods do not detect them.

5. Field-role check. Why can the same BF phase describe an invertible response in one use and a noninvertible dynamical theory in another?

Solution

With AA and BB fixed, each background configuration is assigned one nonzero phase, whose stacking inverse is its complex conjugate. When both fields are integrated, the theory acquires nontrivial sums, operators, and state spaces; in three dimensions dimH(T2)=N2\dim\mathcal H(T^2)=N^2, so N>1N>1 cannot be invertible.

6. Boundary check. What must be added to the statement “BdAB\wedge\mathrm dA is gauge invariant” when MM has a boundary?

Solution

Under BB+dΛB\mapsto B+\mathrm d\Lambda, the action changes by iN2πMΛdA\frac{iN}{2\pi}\int_{\partial M}\Lambda\wedge\mathrm dA. One must specify restricted boundary transformations, a boundary condition or polarization, a compensating counterterm, or boundary degrees of freedom. The arbitrary variation also has a separate BδAB\wedge\delta A boundary term.

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  • Bergeron, M., G. W. Semenoff, and R. J. Szabo. “Canonical BF-Type Topological Field Theory and Fractional Statistics of Strings.” Nuclear Physics B 437 (1995), 695–722. DOI. Open PDF, arXiv:hep-th/9407020v1.
  • Brennan, T. Daniel, and Sungwoo Hong. “Introduction to Generalized Global Symmetries in QFT and Particle Physics.” arXiv:2306.00912v2 (2023), revised 2 June 2023. Stable record.
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