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Antiferromagnets, Spin Chains, and Theta Terms

The previous page solved the two-dimensional O(N)O(N) nonlinear sigma model at large NN and found a mass gap. That result is the right generic expectation for the O(3)O(3) model too: the coupling is asymptotically free, grows in the infrared, and usually produces a finite correlation length. But the O(3)O(3) model has a special extra ingredient in two Euclidean dimensions. Its fields are maps from spacetime into a sphere, and such maps have an integer winding number. The action can therefore contain a theta term.

The Berry phases of microscopic spins determine this term. We derive the leading long-wavelength, large-SS description of the uniform nearest-neighbor chain, then separate its bulk predictions from the additional hypotheses needed for boundary spins and infrared phases. The resulting action is not merely

Skin=12g∫d2x ∂μn⋅∂μn,n2=1,S_{\rm kin}={1\over 2g}\int d^2x\,\partial_\mu\mathbf n\cdot\partial_\mu\mathbf n, \qquad \mathbf n^2=1,

but rather

SE[n]=12g∫d2x ∂μn⋅∂μn+iθQ[n].S_E[\mathbf n] ={1\over 2g}\int d^2x\,\partial_\mu\mathbf n\cdot\partial_\mu\mathbf n +i\theta Q[\mathbf n].

Here Q∈ZQ\in\mathbb Z is the degree of a smooth map n:spacetime→S2\mathbf n:\text{spacetime}\to S^2 when Euclidean spacetime is closed. For the uniform spin-SS antiferromagnetic chain,

θ=2πS.\boxed{\theta=2\pi S.}

Thus integer and half-integer spin chains land at different points on the theta circle:

S∈Z⇒θ=0(mod2π),S\in\mathbb Z\quad\Rightarrow\quad \theta=0\pmod {2\pi},

whereas

S∈Z+12⇒θ=π(mod2π).S\in\mathbb Z+{1\over2}\quad\Rightarrow\quad \theta=\pi\pmod {2\pi}.

This is the continuum-field-theory origin of Haldane’s distinction between integer and half-integer antiferromagnetic spin chains.

For readers coming from relativistic QFT, the important conceptual point is that θ\theta is not chosen by hand in the spin-chain problem. It is fixed by the microscopic spin representation. Changing SS by 1/21/2 changes the interference among topological sectors by a sign.

Required background. Nonlinear sigma models and constraints supplies the O(3)O(3) kinetic theory, and the large-N saddle explains why the model is generically massive without a topological term. Only the coherent-state Berry phase is new here.

Theta-term normalization and spin-chain dictionary

Section titled “Theta-term normalization and spin-chain dictionary”

For the nearest-neighbor antiferromagnetic chain, fix the microscopic spacing aa, exchange JJ, physical Euclidean time, and unit field n\mathbf n. The leading large-SS dictionary is

Lattice quantityContinuum meaning
coherent-state spin direction(−1)jn1−a2ℓ2/S2+(a/S)ℓ(-1)^j\mathbf n\sqrt{1-a^2\boldsymbol\ell^2/S^2}+(a/S)\boldsymbol\ell
n2=1\mathbf n^2=1staggered Néel direction
ℓ⊥n\boldsymbol\ell\perp\mathbf nsmooth uniform magnetization density
c∼2JSac\sim 2JSaspin-wave velocity
g∼2/Sg\sim 2/Ssigma-model coupling at large SS
θ=2πS\theta=2\pi SBerry-phase/topological angle

A consistent rescaling of the auxiliary canting field cancels from the Gaussian integral and does not change these matched cc and gg. The approximation requires slow variation on the scale aa and a∣ℓ∣/S≪1a\lvert\boldsymbol\ell\rvert/S\ll1; large SS controls the semiclassical expansion. Small-SS infrared statements need additional field-theory or microscopic evidence. The original large-spin reduction is developed in Haldane 1983, pp. 1153–1154, Eqs. (5)–(10), PDF.

From a Néel chain to a slowly varying field

Section titled “From a Néel chain to a slowly varying field”

Start with an even periodic antiferromagnetic Heisenberg chain, with sites j=0,…,Ns−1j=0,\ldots,N_{\rm s}-1,

H=J∑jSj⋅Sj+1,J>0,H=J\sum_j \mathbf S_j\cdot\mathbf S_{j+1}, \qquad J>0,

with spin length

Sj2=S(S+1).\mathbf S_j^2=S(S+1).

Classically, the lowest-energy pattern alternates:

↑↓↑↓⋯ .\uparrow\downarrow\uparrow\downarrow\cdots.

The correct slow variable is therefore not the uniform magnetization, but the staggered Néel field n(x,τ)\mathbf n(x,\tau). For a coherent-state unit vector Nj\mathbf N_j, a length-preserving decomposition is

Nj(τ)=(−1)jn(xj,τ)1−a2ℓ2S2+aSℓ(xj,τ),xj=ja,\mathbf N_j(\tau) =(-1)^j\mathbf n(x_j,\tau) \sqrt{1-{a^2\boldsymbol\ell^2\over S^2}} +{a\over S}\boldsymbol\ell(x_j,\tau), \qquad x_j=ja,

where

n2=1,n⋅ℓ=0.\mathbf n^2=1, \qquad \mathbf n\cdot\boldsymbol\ell=0.

The coherent-state expectation value is ⟨Sj⟩=SNj\langle\mathbf S_j\rangle=S\mathbf N_j. Expanding the square root gives the familiar leading shorthand

⟨Sj⟩=S(−1)jn+aℓ+O(a2ℓ2/S).\langle\mathbf S_j\rangle =S(-1)^j\mathbf n+a\boldsymbol\ell+O(a^2\boldsymbol\ell^2/S).

The field n\mathbf n records the local staggered direction. The smaller field ℓ\boldsymbol\ell records the smooth ferromagnetic canting, or uniform magnetization density. The two constraints ensure Nj2=1\mathbf N_j^2=1; the square-root correction matters when deriving coefficients consistently beyond leading order. The figure shows this local orthogonality separately from the alternating microscopic pattern; it does not assume long-range Néel order in the quantum ground state.

Alternating microscopic spins are resolved into a unit staggered direction and a perpendicular small canting field at the same point

The length-preserving decomposition uses a unit staggered field n(x)\mathbf n(x) and a small uniform magnetization density ℓ(x)\boldsymbol\ell(x) tangent to its sphere. The local arrows share one marked point and satisfy n⋅ℓ=0\mathbf n\cdot\boldsymbol\ell=0. This is a schematic separation of slow fields, not a ground-state spin configuration or a scale drawing.

To obtain the coefficients, use n⋅∂xn=0\mathbf n\cdot\partial_x\mathbf n=0 and n⋅∂x2n=−(∂xn)2\mathbf n\cdot\partial_x^2\mathbf n=-(\partial_x\mathbf n)^2. For two neighboring sites, the two square-root corrections and the explicit canting product contribute 2a2ℓ2/S22a^2\boldsymbol\ell^2/S^2. A single bond also has an alternating mixed term; averaging the two bonds of an even cell cancels that term at this order. With the slow fields evaluated at the cell center,

12∑j=2r2r+1Nj⋅Nj+1=−1+2a2ℓ2S2+a22(∂xn)2+⋯ .{1\over2}\sum_{j=2r}^{2r+1}\mathbf N_j\cdot\mathbf N_{j+1} =-1+{2a^2\boldsymbol\ell^2\over S^2} +{a^2\over2}(\partial_x\mathbf n)^2+\cdots.

Dropping the constant and using ∑j→a−1∫dx\sum_j\to a^{-1}\int dx gives the continuum Hamiltonian density

H=2Ja ℓ2+JS2a2(∂xn)2+higher-order terms.\mathcal H =2Ja\,\boldsymbol\ell^2+{JS^2a\over2}(\partial_x\mathbf n)^2+\text{higher-order terms}.

The first term says that uniform canting costs energy. The second term says that spatial gradients of the Néel field cost stiffness. The antiferromagnet is special because the time derivative of n\mathbf n does not come from the microscopic Hamiltonian alone. It comes from the Berry phase of spin coherent states.

A spin-SS coherent state ∣N⟩|\mathbf N\rangle is labeled by a unit vector N∈S2\mathbf N\in S^2 and satisfies

⟨N∣S∣N⟩=SN.\langle \mathbf N|\mathbf S|\mathbf N\rangle=S\mathbf N.

The sign follows from the ordered short-time overlap, rather than from a choice between two equivalent-looking phase factors. For spin 1/21/2, take the north-patch state

∣N⟩=(cos⁡(ϑ/2)eiφsin⁡(ϑ/2)),⟨N∣∂τN⟩=i2(1−cos⁡ϑ)∂τφ.|\mathbf N\rangle= \begin{pmatrix}\cos(\vartheta/2)\\e^{i\varphi}\sin(\vartheta/2)\end{pmatrix}, \qquad \langle\mathbf N|\partial_\tau\mathbf N\rangle ={i\over2}(1-\cos\vartheta)\partial_\tau\varphi.

In Tr⁡e−βH\operatorname{Tr}e^{-\beta H}, successive resolutions of the identity give

⟨N(τ+dτ)∣N(τ)⟩=1−dτ ⟨N∣∂τN⟩+O(dτ2).\langle\mathbf N(\tau+d\tau)|\mathbf N(\tau)\rangle =1-d\tau\,\langle\mathbf N|\partial_\tau\mathbf N\rangle+O(d\tau^2).

A spin-SS coherent state is the symmetric product of 2S2S spinors, so its overlap has 2S2S times this phase. For a closed trajectory, define the positively oriented solid angle by Ω=∮(1−cos⁡ϑ) dφ\Omega=\oint(1-\cos\vartheta)\,d\varphi. The resulting phase is

exp⁡[−iSΩ[N]].\exp\left[-iS\Omega[\mathbf N]\right].

Because the path-integral weight is e−SEe^{-S_E}, the corresponding term in the Euclidean action is

SE,B[N]=+iSΩ[N]=+iS∫dτ A(N)⋅∂τN,S_{E,B}[\mathbf N] =+iS\Omega[\mathbf N] =+iS\int d\tau\,\mathbf A(\mathbf N)\cdot\partial_\tau\mathbf N,

where A\mathbf A is a monopole vector potential on S2S^2 satisfying

∇N×A=N.\nabla_{\mathbf N}\times\mathbf A=\mathbf N.

This formula is local only in patches on the sphere. The solid angle is defined modulo 4π4\pi, so the phase is well-defined precisely because 2S2S is an integer:

e−iS(Ω+4π)=e−iSΩe−i4πS=e−iSΩ.e^{-iS(\Omega+4\pi)}=e^{-iS\Omega}e^{-i4\pi S}=e^{-iS\Omega}.

The overlap construction agrees with Altland and Simons 2023, § 8.4.5, pp. 449–451, Eqs. (8.21)–(8.26): their Euler-gauge state becomes this north-patch state after multiplication by eiSφe^{iS\varphi}. This adds iS∂τφiS\partial_\tau\varphi to their connection −iScos⁡ϑ ∂τφ-iS\cos\vartheta\,\partial_\tau\varphi. The figure fixes the orientation by a positive latitude traversal.

A positively traversed latitude bounds a north-pole cap of solid angle Omega and contributes the Euclidean phase exp minus i S Omega

The positively traversed latitude at ϑ=π/3\vartheta=\pi/3 bounds the displayed north-pole cap, with Ω=2π(1−cos⁡ϑ)=π\Omega=2\pi(1-\cos\vartheta)=\pi. Ordered Euclidean overlaps contribute e−iSΩe^{-iS\Omega}, equivalently the action +iSΩ+iS\Omega; the spin-half phase in this example is −i-i. This north-pole projection is schematic; the solid-angle formula is exact. The ambiguity Ω∼Ω+4π\Omega\sim\Omega+4\pi is harmless because 2S∈Z2S\in\mathbb Z.

For a whole spin chain, the coherent-state path integral contains

exp⁡[−iS∑jΩ[Nj]],\exp\left[-iS\sum_j\Omega[\mathbf N_j]\right],

where Nj(τ)\mathbf N_j(\tau) is the direction of the spin at site jj. In an antiferromagnet,

Nj(τ)≈(−1)jn(xj,τ)+aSℓ(xj,τ).\mathbf N_j(\tau)\approx(-1)^j\mathbf n(x_j,\tau)+{a\over S}\boldsymbol\ell(x_j,\tau).

For positive target curvature the variation is δΩ=∫dτ δn⋅(∂τn×n)\delta\Omega=\int d\tau\,\delta\mathbf n\cdot(\partial_\tau\mathbf n\times\mathbf n). Inserting δNj=(a/S)ℓ\delta\mathbf N_j=(a/S)\boldsymbol\ell around either +n+\mathbf n or −n-\mathbf n gives the same contribution, −(a/S)ℓ⋅(n×∂τn)-(a/S)\boldsymbol\ell\cdot(\mathbf n\times\partial_\tau\mathbf n). Multiplication by +iS+iS and summation over sites therefore give

SE,Bsmooth=−i∫dτ dx ℓ⋅(n×∂τn).S_{E,B}^{\rm smooth}=-i\int d\tau\,dx\, \boldsymbol\ell\cdot(\mathbf n\times\partial_\tau\mathbf n).

Combining this with the continuum Hamiltonian density gives, to leading order,

SE[n,ℓ]=∫dτ dx [2Ja ℓ2+JS2a2(∂xn)2−iℓ⋅(n×∂τn)]+iθQ[n].S_E[\mathbf n,\boldsymbol\ell] =\int d\tau\,dx\, \left[ 2Ja\,\boldsymbol\ell^2 +{JS^2a\over2}(\partial_x\mathbf n)^2 -i\boldsymbol\ell\cdot(\mathbf n\times\partial_\tau\mathbf n) \right] +i\theta Q[\mathbf n].

The field ℓ\boldsymbol\ell is Gaussian. Integrating it out gives

Skin=∫dτ dx [18Ja(∂τn)2+JS2a2(∂xn)2].S_{\rm kin} =\int d\tau\,dx\, \left[{1\over8Ja}(\partial_\tau\mathbf n)^2 +{JS^2a\over2}(\partial_x\mathbf n)^2 \right].

At fixed n\mathbf n, integrate over the two real tangent components of ℓ\boldsymbol\ell. For J>0J>0 this is a convergent Gaussian. Completing the square gives the imaginary stationary point ℓ⋆=i(n×∂τn)/(4Ja)\boldsymbol\ell_\star=i(\mathbf n\times\partial_\tau\mathbf n)/(4Ja) and the positive time-derivative term above; the contour translation is justified by the entire Gaussian integrand and its decay. The field-independent determinant cancels in normalized observables.

This can be written in relativistic-looking form

Skin=12g∫dτ dx [1c(∂τn)2+c(∂xn)2],S_{\rm kin} ={1\over2g}\int d\tau\,dx\, \left[{1\over c}(\partial_\tau\mathbf n)^2+c(\partial_x\mathbf n)^2\right],

with

g=2S,c=2JSa.\boxed{ g={2\over S}, \qquad c=2JSa. }

These are the leading large-SS coefficients for the stated microscopic normalization; see Fradkin 2013, § 7.5, pp. 202–204, Eqs. (7.57)–(7.71). After setting x0=cτx^0=c\tau, this becomes the ordinary two-dimensional O(3)O(3) nonlinear sigma model,

Skin=12g∫d2x (∂μn)2.S_{\rm kin}={1\over2g}\int d^2x\,(\partial_\mu\mathbf n)^2.

The remaining, alternating part of the Berry phase is the topological term. It is here that the microscopic spin length survives in a way no local gradient expansion could guess.

Ferromagnets and antiferromagnets use Berry phases differently

Section titled “Ferromagnets and antiferromagnets use Berry phases differently”

For a ferromagnet, neighboring spins point in nearly the same direction, so their Berry phases add. The continuum Euclidean action begins schematically as

SEferro=+iSa∫dτ dx A(n)⋅∂τn+ρs2∫dτ dx (∂xn)2.S_E^{\rm ferro} =+i{S\over a}\int d\tau\,dx\, \mathbf A(\mathbf n)\cdot\partial_\tau\mathbf n +{\rho_s\over2}\int d\tau\,dx\,(\partial_x\mathbf n)^2.

The time derivative is first order. After continuation to real time, it pairs the two transverse spin-wave coordinates as conjugate variables and gives the quadratic magnon dispersion ω∝k2\omega\propto k^2.

For an antiferromagnet, the leading Berry phases alternate and nearly cancel. Their smooth remainder couples ℓ\boldsymbol\ell to n×∂τn\mathbf n\times\partial_\tau\mathbf n; integrating out the costly canting field ℓ\boldsymbol\ell produces (∂τn)2(\partial_\tau\mathbf n)^2. The semiclassical dispersion is therefore linear, ω≃c∣k∣\omega\simeq c|k|. The cancellation is not complete: its quantized remainder is the theta term derived next.

The Berry phase is sensitive to the fact that neighboring antiferromagnetic spins live near opposite points on the sphere. Pair neighboring sites. The Berry phases of the two spins nearly cancel, but their small mismatch is a total derivative in field space. Summed over the chain, these mismatches become the winding number of the map n(τ,x)\mathbf n(\tau,x).

Varying the north-patch one-form and integrating its ∂τδφ\partial_\tau\delta\varphi term by parts gives

δΩ[n]=∫dτ δn⋅(∂τn×n)=∫dτ sin⁡ϑ(δϑ ∂τφ−∂τϑ δφ).\delta\Omega[\mathbf n] =\int d\tau\, \delta\mathbf n\cdot(\partial_\tau\mathbf n\times\mathbf n) =\int d\tau\,\sin\vartheta \left(\delta\vartheta\,\partial_\tau\varphi -\partial_\tau\vartheta\,\delta\varphi\right).

Taking δn=a∂xn\delta\mathbf n=a\partial_x\mathbf n gives

Ω[n(x+a)]−Ω[n(x)]=a∫dτ ∂xn⋅(∂τn×n)+O(a2).\Omega[\mathbf n(x+a)]-\Omega[\mathbf n(x)] =a\int d\tau\, \partial_x\mathbf n\cdot(\partial_\tau\mathbf n\times\mathbf n)+O(a^2).

Using cyclic symmetry of the scalar triple product,

∂xn⋅(∂τn×n)=−n⋅(∂τn×∂xn).\partial_x\mathbf n\cdot(\partial_\tau\mathbf n\times\mathbf n) =-\mathbf n\cdot(\partial_\tau\mathbf n\times\partial_x\mathbf n).

Use Ω[−n]=−Ω[n]\Omega[-\mathbf n]= -\Omega[\mathbf n] modulo 4π4\pi. An even site and its following odd neighbor contribute Ω[n(x)]−Ω[n(x+a)]\Omega[\mathbf n(x)]-\Omega[\mathbf n(x+a)], the negative of the difference above. There is one such pair per length 2a2a, so

∑j(−1)jΩ[n(xj)]⟶12∫dτ dx n⋅(∂τn×∂xn),SE,Bstaggered=i(2πS)Q[n]mod 2πi.\begin{aligned} \sum_j(-1)^j\Omega[\mathbf n(x_j)] &\longrightarrow {1\over2}\int d\tau\,dx\, \mathbf n\cdot(\partial_\tau\mathbf n\times\partial_x\mathbf n),\\ S_{E,B}^{\rm staggered}&=i(2\pi S)Q[\mathbf n] \quad\text{mod }2\pi i. \end{aligned}

The arrow denotes the leading gradient limit; higher-gradient corrections have been dropped. Thus the Euclidean action contains +iθQ+i\theta Q, with

θ=2πS.\boxed{\theta=2\pi S.}

For the uniform chain, the coefficient is fixed by the quantized microscopic spin representation. Choosing the other sublattice for n\mathbf n reverses QQ and the corresponding theta convention; keep the termination as well when comparing open chains. The continuum phase remembers whether the microscopic spin is integer or half-integer, even though the kinetic coefficients alone do not encode that parity.

Before using the theta term, it is worth seeing why QQ is an integer. Start with the simpler O(2)O(2) case. A path on a circle may be written as

n(t)=eiφ(t),0≤t≤2π,n(t)=e^{i\varphi(t)}, \qquad 0\le t\le 2\pi,

with periodicity of the physical point

n(2π)=n(0).n(2\pi)=n(0).

The angle itself may wind:

φ(2π)=φ(0)+2πk,k∈Z.\varphi(2\pi)=\varphi(0)+2\pi k, \qquad k\in\mathbb Z.

The winding number is

q=12π∫02πdt dφdt=k.q={1\over2\pi}\int_0^{2\pi}dt\,{d\varphi\over dt}=k.

The O(3)O(3) topological charge is the two-dimensional version of this statement. On the Euclidean plane, impose n(x)→n∞\mathbf n(x)\to\mathbf n_\infty at infinity and sufficient regularity for the field to extend smoothly to the one-point compactification,

R2∪{∞}≃S2.\mathbb R^2\cup\{\infty\}\simeq S^2.

Finite action alone does not imply this boundary condition. For example, a field that equals (sin⁡log⁡log⁡r,0,cos⁡log⁡log⁡r)(\sin\log\log r,0,\cos\log\log r) for r>er>e, smoothly completed inside, has a finite energy tail proportional to ∫R∞dr/[r(log⁡r)2]=1/log⁡R\int_R^\infty dr/[r(\log r)^2]=1/\log R, yet has no limit at infinity. With the stated compactification hypothesis, a field configuration is a map

n:Sspacetime2→Starget2.\mathbf n:S^2_{\rm spacetime}\to S^2_{\rm target}.

Such maps have an integer degree. In angular coordinates on the target sphere,

n=(sin⁡Θcos⁡Φ,sin⁡Θsin⁡Φ,cos⁡Θ),\mathbf n=(\sin\Theta\cos\Phi,\sin\Theta\sin\Phi,\cos\Theta),

one finds

n⋅(∂τn×∂xn)=sin⁡Θ ∂(Θ,Φ)∂(τ,x).\mathbf n\cdot(\partial_\tau\mathbf n\times\partial_x\mathbf n) =\sin\Theta\, {\partial(\Theta,\Phi)\over\partial(\tau,x)}.

Therefore

Q=14π∫dτ dx sin⁡Θ ∂(Θ,Φ)∂(τ,x).Q={1\over4\pi}\int d\tau\,dx\, \sin\Theta\,{\partial(\Theta,\Phi)\over\partial(\tau,x)}.

This is the signed target-sphere area swept out by the map, divided by the area 4π4\pi of the unit sphere. For a regular target point, count its preimages with the signs of their local Jacobians. The signed count is the degree; pulling back the sphere’s area form and summing those oriented sheets gives 4π4\pi times that integer. A configuration that covers the target sphere once with positive orientation has Q=1Q=1. The figure shows the domain hypothesis that licenses this interpretation.

A smooth field with a fixed limit at infinity extends from the compactified domain sphere to the target sphere, with integer signed degree Q

With a fixed limiting field and a smooth extension at infinity, the plane becomes a compact domain S2S^2. The degree of n:S2→S2\mathbf n:S^2\to S^2 is the signed target area divided by 4π4\pi. Finite action by itself is insufficient. The spheres and arrow are schematic; the orientation and normalization of QQ are explicit.

On a closed spacetime, the theta term does not change the local classical equations of motion for smooth variations within a fixed topological sector. It multiplies sectors by phases:

Z(θ)=∑Q∈Ze−iθQZQ,Z(\theta)=\sum_{Q\in\mathbb Z}e^{-i\theta Q}Z_Q,

where ZQZ_Q is the contribution from configurations of topological charge QQ. Since QQ is integer on a closed oriented spacetime,

Z(θ+2π)=Z(θ).Z(\theta+2\pi)=Z(\theta).

The statements “QQ is an integer,” “θ\theta is 2π2\pi-periodic,” and “the theta term does not affect the local variation” all require a qualification when spacetime has a boundary. Orient the thermal strip M=[0,β]τ×[xL,xR]M=[0,\beta]_{\tau}\times[x_L,x_R], with τ\tau periodically identified, by dτ∧dxd\tau\wedge dx, as in the bulk convention above, and use the outward-normal-first rule on ∂M\partial M. The left boundary is then traversed with increasing τ\tau, while the right boundary is traversed with decreasing τ\tau. Let ΩL\Omega_L and ΩR\Omega_R denote the solid angles swept by the two endpoint fields when each is parametrized with increasing τ\tau, using the same target-sphere orientation as the single-spin Berry phase above. After attaching orientation-compatible caps, Stokes’ theorem gives

Qstrip=k+ΩL−ΩR4π,k∈Z.Q_{\rm strip} =k+{\Omega_L-\Omega_R\over4\pi}, \qquad k\in\mathbb Z.

The integer kk changes when a different cap is chosen, while the full microscopic Berry factor remains unambiguous. Substituting θ=2πS\theta=2\pi S shows that the boundary-dependent part of the Euclidean action is

Sedge=+iS2ΩL−iS2ΩR.S_{\rm edge} =+i{S\over2}\Omega_L-i{S\over2}\Omega_R.

For an integer-spin chain with a gapped Haldane bulk and the corresponding open termination, these are the Berry actions of two effective spins S/2S/2 with opposite boundary orientations. The right-hand minus sign can be represented by an edge direction −nR-\mathbf n_R. The closed-bulk factor e−i2πSke^{-i2\pi S k} is then trivial, while the edge factors need not be. The open spin-1 valence-bond construction exhibits the spin-1/21/2 endpoints explicitly; see Affleck, Kennedy, Lieb and Tasaki 1987, pp. 799–801, PDF.

The integer-spin hypothesis matters. Changing the left cap sends ΩL→ΩL+4π\Omega_L\to\Omega_L+4\pi and k→k−1k\to k-1, leaving the full QstripQ_{\rm strip} unchanged. The isolated edge factor would instead acquire e−i2πSe^{-i2\pi S}. It is single-valued for integer SS but changes sign for half-integer SS. A gapless spin-half bulk therefore does not supply an autonomous spin-quarter edge: the bulk and boundary expression must be retained together.

The protected information is the projective symmetry class of the edge, rather than a fixed S/2S/2 multiplet for every boundary Hamiltonian. For odd integer SS, the half-integer edge is projective under SO(3)SO(3) and has Kramers degeneracy under physical time reversal. For even integer SS, an integer-spin boundary multiplet can be screened or replaced by a singlet without closing the bulk gap. These statements assume the protecting symmetry and a gapped bulk; Pollmann, Berg, Turner and Oshikawa 2012, arXiv v3, § III.A, pp. 3–4, PDF explains the edge-level distinction.

This resolves an apparent contradiction. The bulk values θ=0\theta=0 and θ=2π\theta=2\pi give the same partition function on a closed spacetime, yet they can encode different boundary physics when the protecting symmetries are retained. Theta periodicity should therefore never be used to erase an open chain’s boundary Berry phases.

Combining

θ=2πS\theta=2\pi S

with closed-spacetime theta periodicity gives two possible topological phases in the microscopic weight:

S∈Z⇒θ=0(mod2π),S∈Z+12⇒θ=π(mod2π).\begin{array}{ccl} S\in\mathbb Z &\Rightarrow& \theta=0\pmod{2\pi},\\ S\in\mathbb Z+{1\over2} &\Rightarrow& \theta=\pi\pmod{2\pi}. \end{array}

At θ=0\theta=0, the closed-bulk O(3)O(3) model behaves like the ordinary asymptotically free sigma model. The coupling grows in the infrared and the theory produces a mass gap,

M∼Λe−2π/g,M\sim \Lambda e^{-2\pi/g},

up to prefactors and scheme-dependent definitions of the ultraviolet scale. For the uniform nearest-neighbor chain and its Haldane phase, this gives the leading semiclassical explanation of the integer-spin bulk gap. It is not a proof of the microscopic gap for every SS from the gradient expansion. The bulk statement also does not remove the boundary degrees of freedom of an open chain.

At θ=π\theta=\pi, the topological sectors enter with the sign

e−iπQ=(−1)Q.e^{-i\pi Q}=(-1)^Q.

Even and odd sectors enter with opposite signs; this does not imply that their magnitudes cancel exactly. For the uniform nearest-neighbor spin-1/21/2 Heisenberg antiferromagnet, the infrared fixed point is the SU(2)1SU(2)_1 Wess–Zumino–Witten conformal field theory, with logarithmic corrections from a marginally irrelevant operator. In a one-dimensional spin system with finite-range interactions at zero temperature in the thermodynamic limit, the Lieb–Schultz–Mattis constraint rules out a unique symmetry-preserving gapped ground state with half-odd-integer spin per unit cell and unbroken one-site translation and spin-rotation symmetry. A gapless phase and symmetry-breaking ground-state degeneracy are distinct alternatives; the theta angle alone does not select between all possible microscopic Hamiltonians. See Affleck and Haldane 1987, pp. 5294 and 5297, PDF.

The figure separates this uniform-chain classification from the effect of explicit bond alternation discussed next. Its arrows express the stated implications, not trajectories in a computed coupling plane.

Uniform integer and half-integer chains fix closed-bulk theta to zero and pi respectively, while explicit dimerization removes the one-site translation restriction

For the uniform chain, the microscopic spin fixes θ=2πS\theta=2\pi S; periodicity reduces it to 00 or π\pi on closed spacetime. The ordinary θ=0\theta=0 sigma model is massive, and the nearest-neighbor spin-half chain at θ=π\theta=\pi is critical. More general half-integer chains obey the symmetry obstruction stated in the text. Explicit dimerization breaks one-site translation while preserving physical time reversal and can open a gap. This is a schematic classification, not an RG-flow calculation; open-chain edges require the separate boundary action.

This is a striking lesson. The local Lagrangian density

12g(∂n)2{1\over2g}(\partial\mathbf n)^2

has the same local form for S=1S=1 and S=1/2S=1/2, although its matched coupling gg differs. It does not encode the quantized integer/half-integer interference. That information lies in a topological phase invisible in ordinary perturbation theory around a smooth trivial-sector configuration.

The antiferromagnetic chain has microscopic symmetries that act nontrivially on the continuum field. A one-site translation reverses the Néel field:

Ta:n↦−n.T_a:\quad \mathbf n\mapsto -\mathbf n.

The topological density changes sign under this map because

(−n)⋅[∂τ(−n)×∂x(−n)]=−n⋅(∂τn×∂xn),(-\mathbf n)\cdot[\partial_\tau(-\mathbf n)\times\partial_x(-\mathbf n)] =-\mathbf n\cdot(\partial_\tau\mathbf n\times\partial_x\mathbf n),

so

Q↦−Q.Q\mapsto -Q.

Because translation is unitary, the path-integral phase can be invariant under this transformation only when

e−iθQ=eiθQfor all Q∈Z,e^{-i\theta Q}=e^{i\theta Q} \qquad \text{for all }Q\in\mathbb Z,

which requires

θ=0orθ=π(mod2π).\theta=0\quad\text{or}\quad \theta=\pi\pmod{2\pi}.

These two symmetry-invariant values are precisely the two values realized by uniform integer and half-integer antiferromagnetic spin chains.

Physical time reversal reverses spins and the temporal ordering of a history. For an antiunitary operator T\mathcal T,

⟨Tu∣Tv⟩=⟨v∣u⟩.\langle\mathcal T u|\mathcal T v\rangle=\langle v|u\rangle.

For a periodic sequence of states uju_j, set uj′=TuM−ju'_j=\mathcal T u_{M-j}. Each transformed overlap is ⟨uj+1′∣uj′⟩=⟨uM−j∣uM−j−1⟩\langle u'_{j+1}|u'_j\rangle=\langle u_{M-j}|u_{M-j-1}\rangle, so the cyclic product is unchanged. Complex conjugating this reversed product once more would count the reversal twice. The corresponding field history is n′(τ,x)=−n(−τ,x)\mathbf n'(\tau,x)=-\mathbf n(-\tau,x); its topological density is qtop′(τ,x)=qtop(−τ,x)q'_{\rm top}(\tau,x)=q_{\rm top}(-\tau,x). Physical spin time reversal therefore does not impose the same restriction on θ\theta as unitary one-site translation.

A concrete check is the spin-half alternating chain

Hδ=J∑j[1+(−1)jδ] Sj⋅Sj+1,∣δ∣<1.H_\delta=J\sum_j[1+(-1)^j\delta]\,\mathbf S_j\cdot\mathbf S_{j+1}, \qquad |\delta|<1.

Every exchange product is time-reversal invariant, for any real δ\delta. One-site translation instead sends δ→−δ\delta\to-\delta. With even bonds chosen strong for δ>0\delta>0, the alternating mixed bond term no longer cancels. At the same gradient order the Hamiltonian density is

Hδ=2Ja ℓ2−2JSaδ ℓ⋅∂xn+JS2a2(∂xn)2.\mathcal H_\delta =2Ja\,\boldsymbol\ell^2 -2JSa\delta\,\boldsymbol\ell\cdot\partial_x\mathbf n +{JS^2a\over2}(\partial_x\mathbf n)^2.

Shift the real tangent field by ℓ=ℓ~+(Sδ/2)∂xn\boldsymbol\ell=\widetilde{\boldsymbol\ell}+(S\delta/2)\partial_x\mathbf n. Its Berry coupling then leaves the extra action −i(Sδ/2)∫dτ dx n⋅(∂τn×∂xn)-i(S\delta/2)\int d\tau\,dx\,\mathbf n\cdot(\partial_\tau\mathbf n\times\partial_x\mathbf n). Combining it with +i2πSQ+i2\pi SQ gives θ=2πS(1−δ)\theta=2\pi S(1-\delta) at this matching order. For spin half,

SE,θ=iπ(1−δ)Q,θ=π(1−δ).S_{E,\theta}=i\pi(1-\delta)Q, \qquad \theta=\pi(1-\delta).

This follows from Foussats, Greco and Muramatsu 2011, § 4, pp. 235–239, Eqs. (4.1), (4.22)–(4.24), PDF. Their topological integral is 4πQ4\pi Q in our normalization, so its coefficient i(1−δ)/4i(1-\delta)/4 gives the expression above. For example, δ=1/2\delta=1/2 preserves physical time reversal while giving θ=π/2\theta=\pi/2. Bond alternation is relevant near the uniform spin-half critical chain and opens a gap; the doubled cell contains integer total spin, so the one-site Lieb–Schultz–Mattis obstruction no longer applies. This continuum matching does not by itself determine the gap at arbitrary strong dimerization.

Locally, the O(3)O(3) field has only two independent components. Choose a patch near the north pole and write

n=(1−π2,π1,π2),π2=π12+π22.\mathbf n=(\sqrt{1-\boldsymbol\pi^2},\pi_1,\pi_2), \qquad \boldsymbol\pi^2=\pi_1^2+\pi_2^2.

Then

(∂μn)2=(∂μπ)2+(π⋅∂μπ)21−π2.(\partial_\mu\mathbf n)^2 =(\partial_\mu\boldsymbol\pi)^2 +{(\boldsymbol\pi\cdot\partial_\mu\boldsymbol\pi)^2\over1-\boldsymbol\pi^2}.

So the two local fields π1,π2\pi_1,\pi_2 are the spin-wave coordinates. At weak coupling, after rescaling π=g φ\boldsymbol\pi=\sqrt g\,\boldsymbol\varphi, the leading interaction is order gg. This is the same perturbative sigma-model expansion used on the previous pages.

The topological term is different. In a single coordinate patch, it looks like a total derivative or a curl. On a closed spacetime it does not change the perturbative beta function of gg at any finite order. With a boundary, the same total derivative is precisely why a boundary term remains. Globally, no single smooth coordinate patch covers all configurations of nonzero QQ. The theta term can therefore be invisible in bulk perturbation theory and still decide the infrared and edge physics.

The continuum antiferromagnet raises a question that sounds paradoxical at first. The microscopic classical picture has a Néel vector, but the one-dimensional quantum chain has no ordinary long-range staggered magnetization in its symmetric ground state. In field-theory language, low-dimensional fluctuations restore the continuous symmetry.

The next page studies this symmetry restoration more directly. It returns to the sigma model as a quantum field theory and explains why the order parameter vanishes even when the classical field wants to choose a point on the sphere.

A one-dimensional antiferromagnetic Heisenberg spin chain has low-energy variables

Sj≈S(−1)jn(xj)+aℓ(xj),n2=1,n⋅ℓ=0.\mathbf S_j\approx S(-1)^j\mathbf n(x_j)+a\boldsymbol\ell(x_j), \qquad \mathbf n^2=1, \qquad \mathbf n\cdot\boldsymbol\ell=0.

The exchange interaction gives spatial stiffness and a cost for uniform canting. The spin coherent-state Berry phase gives the time derivative term and, more importantly, the theta term. After integrating out ℓ\boldsymbol\ell, the low-energy Euclidean action is

SE[n]=12g∫dτ dx [1v(∂τn)2+v(∂xn)2]+iθQ[n],S_E[\mathbf n] ={1\over2g}\int d\tau\,dx\, \left[{1\over v}(\partial_\tau\mathbf n)^2+v(\partial_x\mathbf n)^2\right] +i\theta Q[\mathbf n],

with

g=2S,v=2JSa,θ=2πS.g={2\over S}, \qquad v=2JSa, \qquad \theta=2\pi S.

The topological charge is

Q=14π∫dτ dx n⋅(∂τn×∂xn)∈Zon closed spacetime.Q={1\over4\pi}\int d\tau\,dx\, \mathbf n\cdot(\partial_\tau\mathbf n\times\partial_x\mathbf n) \in\mathbb Z \qquad\text{on closed spacetime}.

Thus integer spin gives θ=0\theta=0 modulo 2π2\pi and the ordinary massive bulk sigma-model behavior, while half-integer spin gives θ=π\theta=\pi modulo 2π2\pi. The nearest-neighbor spin-1/21/2 chain is critical; more generally, the half-odd-integer chain cannot be a trivial unique symmetric gapped state. On an open chain, the bulk periodicity must be supplemented by the endpoint Berry phases, which retain information that a closed-spacetime reduction θ∼θ+2π\theta\sim\theta+2\pi would discard.

Forgetting the Berry phase. The ordinary gradient energy only produces the sigma-model kinetic term. The integer versus half-integer distinction comes from the spin coherent-state Berry phase.

Mixing the Berry factor with the Euclidean action. With the positive-curvature solid angle used here, ordered coherent-state overlaps give e−iSΩe^{-iS\Omega} and the Euclidean action is +iSΩ+iS\Omega. Derive the variation and the canting coupling using that same orientation.

Treating the theta term as a small local perturbation. It weights entire topological sectors by phases e−iθQe^{-i\theta Q}. Its leading density can be a total derivative in one patch while its global effect remains nonperturbative.

Losing the factor of 2π2\pi. The spin-chain result is θ=2πS\theta=2\pi S, not θ=S\theta=S. Since θ\theta is periodic modulo 2π2\pi on closed spacetime, this factor is exactly what separates integer from half-integer bulk theories.

Using closed-spacetime periodicity on an open chain. When there is a boundary, QQ need not be an integer by itself and the theta term leaves endpoint Berry phases. In particular, reducing θ=2π\theta=2\pi to zero before retaining the boundary term erases the spin-1/21/2 edges of the spin-1 Haldane chain.

Overstating the gapless claim. The uniform nearest-neighbor spin-1/21/2 Heisenberg antiferromagnet is critical, but the general half-odd-integer constraint allows either gaplessness or degeneracy. Explicit dimerization can open a gap because it doubles the unit cell and breaks one-site translation.

Exercise 1: integrating out the uniform magnetization

Section titled “Exercise 1: integrating out the uniform magnetization”

Starting from

SE[n,ℓ]=∫dτ dx [2Ja ℓ2+JS2a2(∂xn)2−iℓ⋅(n×∂τn)],S_E[\mathbf n,\boldsymbol\ell] =\int d\tau\,dx\, \left[ 2Ja\,\boldsymbol\ell^2 +{JS^2a\over2}(\partial_x\mathbf n)^2 -i\boldsymbol\ell\cdot(\mathbf n\times\partial_\tau\mathbf n) \right],

with n2=1\mathbf n^2=1, n⋅ℓ=0\mathbf n\cdot\boldsymbol\ell=0, and J>0J>0, complete the tangent-plane Gaussian square and show that the time-derivative term is

18Ja(∂τn)2.{1\over8Ja}(\partial_\tau\mathbf n)^2.
Solution

The ℓ\boldsymbol\ell-dependent part is

2Ja ℓ2−iℓ⋅A,A=n×∂τn.2Ja\,\boldsymbol\ell^2 -i\boldsymbol\ell\cdot\mathbf A, \qquad \mathbf A=\mathbf n\times\partial_\tau\mathbf n.

The stationary point satisfies

4Ja ℓ−iA=0,4Ja\,\boldsymbol\ell-i\mathbf A=0,

so

ℓ⋆=i4JaA.\boldsymbol\ell_\star={i\over4Ja}\mathbf A.

Completing the square,

2Ja(ℓ−iA4Ja)2+18JaA2.2Ja\left(\boldsymbol\ell-{i\mathbf A\over4Ja}\right)^2 +{1\over8Ja}\mathbf A^2.

Since n2=1\mathbf n^2=1, we have

n⋅∂τn=0,\mathbf n\cdot\partial_\tau\mathbf n=0,

and therefore

A2=(n×∂τn)2=(∂τn)2.\mathbf A^2=(\mathbf n\times\partial_\tau\mathbf n)^2 =(\partial_\tau\mathbf n)^2.

Thus integrating out ℓ\boldsymbol\ell gives

18Ja(∂τn)2.{1\over8Ja}(\partial_\tau\mathbf n)^2.

Exercise 2: topological charge of the identity map

Section titled “Exercise 2: topological charge of the identity map”

Let the domain sphere have coordinates (ϑ,φ)(\vartheta,\varphi) with 0≤ϑ≤π0\le\vartheta\le\pi and 0≤φ<2π0\le\varphi<2\pi. Consider the identity map to the target sphere,

n(ϑ,φ)=(sin⁡ϑcos⁡φ,sin⁡ϑsin⁡φ,cos⁡ϑ).\mathbf n(\vartheta,\varphi)=(\sin\vartheta\cos\varphi,\sin\vartheta\sin\varphi,\cos\vartheta).

Show that Q=1Q=1.

Solution

For this parameterization,

n⋅(∂ϑn×∂φn)=sin⁡ϑ.\mathbf n\cdot(\partial_\vartheta\mathbf n\times\partial_\varphi\mathbf n)=\sin\vartheta.

Therefore

Q=14π∫0πdϑ∫02πdφ sin⁡ϑ.Q={1\over4\pi}\int_0^\pi d\vartheta\int_0^{2\pi}d\varphi\,\sin\vartheta.

The integrals give

∫0πdϑ sin⁡ϑ=2,∫02πdφ=2π.\int_0^\pi d\vartheta\,\sin\vartheta=2, \qquad \int_0^{2\pi}d\varphi=2\pi.

Thus

Q=14π(2)(2π)=1.Q={1\over4\pi}(2)(2\pi)=1.

The identity map covers the target sphere exactly once with positive orientation.

Exercise 3: the boundary term at θ = 2πS

Section titled “Exercise 3: the boundary term at θ = 2πS”

For an integer-spin chain in a gapped Haldane regime with the open termination described above, suppose the capped topological charge is

Qstrip=k+ΩL−ΩR4π,k∈Z.Q_{\rm strip}=k+{\Omega_L-\Omega_R\over4\pi}, \qquad k\in\mathbb Z.

Insert θ=2πS\theta=2\pi S into Sθ=+iθQstripS_\theta=+i\theta Q_{\rm strip}. Identify the two edge Berry actions and the spin-1 example. Why would separating off an autonomous spin-S/2S/2 edge fail for microscopic S=1/2S=1/2?

Solution

Substitution gives

Sθ=+i2πSk+iS2(ΩL−ΩR).S_\theta =+i2\pi S k +i{S\over2}(\Omega_L-\Omega_R).

The second term is

+iS2ΩL−iS2ΩR.+i{S\over2}\Omega_L-i{S\over2}\Omega_R.

The signs reflect the opposite boundary orientations. For S=1S=1, the bulk factor e−i2πk=1e^{-i2\pi k}=1, while the two endpoints have spin-1/21/2 Berry actions. This identifies their projective edge class in the stated gapped regime. For microscopic S=1/2S=1/2, changing one cap by 4π4\pi multiplies its isolated spin-quarter phase by e−iπ=−1e^{-i\pi}=-1. The compensating change k→k−1k\to k-1 restores the full strip phase, so the separate edge factor is not an autonomous spin path integral.

Exercise 4: translation and the topological charge

Section titled “Exercise 4: translation and the topological charge”

A one-site translation acts on the Néel field as n↦−n\mathbf n\mapsto-\mathbf n. Show that this sends Q↦−QQ\mapsto -Q. For which theta angles is the phase e−iθQe^{-i\theta Q} invariant under this transformation for all Q∈ZQ\in\mathbb Z?

Solution

Under n↦−n\mathbf n\mapsto-\mathbf n,

∂μn↦−∂μn.\partial_\mu\mathbf n\mapsto-\partial_\mu\mathbf n.

The cross product of two derivatives is unchanged:

∂τ(−n)×∂x(−n)=∂τn×∂xn.\partial_\tau(-\mathbf n)\times\partial_x(-\mathbf n) =\partial_\tau\mathbf n\times\partial_x\mathbf n.

But the remaining factor of n\mathbf n changes sign, so

(−n)⋅[∂τ(−n)×∂x(−n)]=−n⋅(∂τn×∂xn).(-\mathbf n)\cdot[\partial_\tau(-\mathbf n)\times\partial_x(-\mathbf n)] =-\mathbf n\cdot(\partial_\tau\mathbf n\times\partial_x\mathbf n).

Therefore

Q↦−Q.Q\mapsto -Q.

The phase is invariant if

e−iθQ=eiθQe^{-i\theta Q}=e^{i\theta Q}

for all integers QQ. This requires

e−i2θQ=1e^{-i2\theta Q}=1

for all QQ, hence

2θ=2πk,k∈Z.2\theta=2\pi k, \qquad k\in\mathbb Z.

Modulo 2π2\pi, the solutions are

θ=0,θ=π.\theta=0, \qquad \theta=\pi.

Exercise 5: why the theta term is invisible in small-field perturbation theory

Section titled “Exercise 5: why the theta term is invisible in small-field perturbation theory”

In a local patch write

n=(1−π12−π22,π1,π2).\mathbf n=(\sqrt{1-\pi_1^2-\pi_2^2},\pi_1,\pi_2).

Count derivatives at the same small-field amplitude order as the fields. Show that the topological density begins with a total derivative:

n⋅(∂τn×∂xn)=∂τπ1∂xπ2−∂τπ2∂xπ1+O(π4).\mathbf n\cdot(\partial_\tau\mathbf n\times\partial_x\mathbf n) =\partial_\tau\pi_1\partial_x\pi_2- \partial_\tau\pi_2\partial_x\pi_1+O(\pi^4).

Then rewrite the leading term as a total derivative and explain what changes when spacetime has a boundary.

Solution

To leading order,

n=(1,π1,π2)+O(π2),\mathbf n=(1,\pi_1,\pi_2)+O(\pi^2),

so

∂τn=(0,∂τπ1,∂τπ2)+O(π2),\partial_\tau\mathbf n=(0,\partial_\tau\pi_1,\partial_\tau\pi_2)+O(\pi^2),

and

∂xn=(0,∂xπ1,∂xπ2)+O(π2).\partial_x\mathbf n=(0,\partial_x\pi_1,\partial_x\pi_2)+O(\pi^2).

The leading cross product points in the first internal direction:

∂τn×∂xn=(∂τπ1∂xπ2−∂τπ2∂xπ1,0,0)+O(π3).\partial_\tau\mathbf n\times\partial_x\mathbf n =\left(\partial_\tau\pi_1\partial_x\pi_2- \partial_\tau\pi_2\partial_x\pi_1,0,0\right)+O(\pi^3).

Dotting with n=(1,π1,π2)+⋯\mathbf n=(1,\pi_1,\pi_2)+\cdots gives

n⋅(∂τn×∂xn)=∂τπ1∂xπ2−∂τπ2∂xπ1+O(π4).\mathbf n\cdot(\partial_\tau\mathbf n\times\partial_x\mathbf n) =\partial_\tau\pi_1\partial_x\pi_2- \partial_\tau\pi_2\partial_x\pi_1+O(\pi^4).

The leading term is

∂τπ1∂xπ2−∂τπ2∂xπ1=∂τ(π1∂xπ2)−∂x(π1∂τπ2),\partial_\tau\pi_1\partial_x\pi_2- \partial_\tau\pi_2\partial_x\pi_1 =\partial_\tau(\pi_1\partial_x\pi_2)-\partial_x(\pi_1\partial_\tau\pi_2),

because mixed derivatives commute. On a closed spacetime, or for fluctuations that vanish at infinity, the integral of this term vanishes. With a boundary it instead leaves a boundary contribution, consistent with the endpoint Berry phases derived above. This is why the theta term does not modify ordinary bulk perturbation theory around the trivial sector while remaining physically important.

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