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Finite-Dimensional and Equivariant Localization

The Atiyah–Bott–Berline–Vergne formula is a theorem about a compact group acting on a finite-dimensional manifold. It replaces the integral of an equivariantly closed form by integrals over the fixed components, weighted by inverse equivariant Euler classes. This is the clean mathematical model for supersymmetric localization. It is not, by itself, a theorem about an infinite-dimensional quantum-field-theory path integral.

Required background. Differential forms, integration, and Stokes’ theorem supplies integration of closed forms. Fredholm and Dirac index theorems supplies the later infinite-dimensional replacement for a normal-bundle Euler class. Lie groups, Lie algebras, and adjoint actions supplies torus actions and weights.

Helpful background. Topological and holomorphic twists motivates why an odd symmetry can act like an equivariant differential.

Let a compact torus TT with Lie algebra t\mathfrak t act smoothly on a manifold MM. Choose a basis eae_a of t\mathfrak t, let VaV_a be the corresponding generating vector fields, and let uau^a be the dual polynomial variables. The Cartan complex is

ΩT(M)=(S(t∗)⊗Ω(M))T,deg⁡ua=2.\Omega_T(M) =\bigl(S(\mathfrak t^*)\otimes\Omega(M)\bigr)^T, \qquad \deg u^a=2.

The total degree is twice the polynomial degree plus the ordinary form degree. In particular,

deg⁡ ⁣((u1)k1⋯(ur)krωp)=2∑aka+p.\deg\!\left((u^1)^{k_1}\cdots(u^r)^{k_r}\omega_p\right) =2\sum_a k_a+p.

With the sign convention used on this page,

dT=d−uaιVa.d_T=d-u^a\iota_{V_a}.

Cartan’s identity gives

dT2=−uaLVa.d_T^2=-u^a\mathcal L_{V_a}.

Therefore dT2=0d_T^2=0 on the TT-invariant complex. An element α(u)\alpha(u) satisfying dTα=0d_T\alpha=0 is equivariantly closed. When MM is oriented and either compact or the form has compact support, equivariant integration means taking the ordinary top-form component and integrating it over MM:

∫M:ΩT(M)⟶S(t∗).\int_M:\Omega_T(M)\longrightarrow S(\mathfrak t^*).

It lowers total degree by dim⁡M\dim M. Rational functions of the uau^a enter only after localizing the coefficient ring.

For a Hamiltonian circle action, this convention is easy to test. If VV preserves a symplectic form ω\omega and

dμ=ιVω,d\mu=\iota_V\omega,

then

ΩT=ω+uμ,dTΩT=u(dμ−ιVω)=0.\Omega_T=\omega+u\mu, \qquad d_T\Omega_T=u\bigl(d\mu-\iota_V\omega\bigr)=0.

Authors who use dT=d+uιVd_T=d+u\iota_V use the opposite sign for the moment-map term. Mixing those two conventions reverses fixed-point exponentials.

Atiyah–Bott–Berline–Vergne formula. Let TT act smoothly on a compact oriented manifold MM without boundary. Let

F=MT=∐iFiF=M^T=\coprod_i F_i

be its fixed set, and let ιi:Fi↪M\iota_i:F_i\hookrightarrow M be the inclusions. Each FiF_i is a smooth closed submanifold. Orient its normal bundle NiN_i consistently with the orientations of MM and FiF_i. For every equivariantly closed α\alpha, after inverting the nonzero torus weights,

∫Mα=∑i∫Fiιi∗αeT(Ni).\int_M\alpha =\sum_i\int_{F_i} \frac{\iota_i^*\alpha}{e_T(N_i)}.

The equality lives in the localized equivariant coefficient ring. The exponential of an equivariant two-form is interpreted coefficient by coefficient, or in the corresponding completed ring. The topological localization theorem and integration formula are given in Atiyah and Bott 1984, §3, especially Eq. (3.8); the differential-form version is developed in their §4. The independent fixed-zero formulation appears in Berline and Vergne 1983, Théorème 1.6.

At an isolated fixed point pp of a 2n2n-dimensional manifold, the tangent representation splits into oriented real two-planes. Let their weights be wp,1,…,wp,n∈t∗w_{p,1},\ldots,w_{p,n}\in\mathfrak t^*. In the convention

eT(TpM)=∏j=1nwp,j2π,e_T(T_pM)=\prod_{j=1}^n\frac{w_{p,j}}{2\pi},

the contribution is

ιp∗αeT(TpM)=(2π)nιp∗α∏jwp,j.\frac{\iota_p^*\alpha}{e_T(T_pM)} =(2\pi)^n \frac{\iota_p^*\alpha}{\prod_j w_{p,j}}.

The factors of 2π2\pi are conventional; the numerator and Euler class must use the same Chern–Weil normalization. A positive-dimensional fixed component remains an integral over that component. Localization does not turn it into an isolated point.

The proof has two distinct ingredients: exactness away from the fixed set and the Thom isomorphism near it.

Choose a generic ξ∈t\xi\in\mathfrak t whose vector field VξV_\xi vanishes precisely on FF. Average a metric over TT, and on M∖FM\setminus F define

λ=g(Vξ, ⋅)∥Vξ∥2.\lambda=\frac{g(V_\xi,\,\cdot)}{\lVert V_\xi\rVert^2}.

Then ιVξλ=1\iota_{V_\xi}\lambda=1. For the evaluated Cartan differential dξ=d−ιVξd_\xi=d-\iota_{V_\xi},

dξλ=dλ−1.d_\xi\lambda=d\lambda-1.

Its ordinary-form-degree-zero part is −1-1, so it has a finite geometric-series inverse. Because λ\lambda is invariant,

dξ ⁣(λdξλ)=1on M∖F.d_\xi\!\left(\frac{\lambda}{d_\xi\lambda}\right)=1 \qquad\text{on }M\setminus F.

Consequently every dξd_\xi-closed form is dξd_\xi exact away from FF. Remove small tubular neighborhoods of the FiF_i and apply Stokes’ theorem. The new boundary terms are converted by the equivariant Thom isomorphism into

ιi∗ιi∗(β)=eT(Ni) β,\iota_i^*\iota_{i*}(\beta)=e_T(N_i)\,\beta,

which explains the inverse Euler class. Compactness and the absence of an original boundary ensure that no additional surface term survives.

This proof also explains why every hypothesis matters. The fixed set of a smooth compact-torus action is already a smooth submanifold, and its normal representation has no trivial TT-weight. If a denominator vanishes after substituting a special ξ\xi, then ξ\xi is nongeneric: its one-parameter subgroup fixes more directions, so one must use the larger fixed set rather than delete the zero factor.

Worked example: rotation of the two-sphere

Section titled “Worked example: rotation of the two-sphere”

Give S2S^2 the orientation and area form

ω=sin⁡θ dθ∧dφ,∫S2ω=4π.\omega=\sin\theta\,d\theta\wedge d\varphi, \qquad \int_{S^2}\omega=4\pi.

Let U(1)U(1) rotate φ\varphi, so V=∂φV=\partial_\varphi. For μ=cos⁡θ\mu=\cos\theta,

ιVω=−sin⁡θ dθ=dμ.\iota_V\omega=-\sin\theta\,d\theta=d\mu.

Hence ΩT=ω+uμ\Omega_T=\omega+u\mu is equivariantly closed. Since ω2=0\omega^2=0 on S2S^2, the ordinary two-form part of eΩTe^{\Omega_T} is euμωe^{u\mu}\omega, and direct integration gives

I(u)=∫S2eΩT=∫02πdφ∫0πeucos⁡θsin⁡θ dθ=4πsinh⁡uu.\begin{aligned} I(u) &=\int_{S^2}e^{\Omega_T}\\ &=\int_0^{2\pi}d\varphi\int_0^\pi e^{u\cos\theta}\sin\theta\,d\theta\\ &=4\pi\frac{\sinh u}{u}. \end{aligned}

The fixed points are the north and south poles. Their moment-map values are +1+1 and −1-1. With the orientation induced by ω\omega, their tangent weights are +u+u and −u-u, so

I(u)=euu/(2π)+e−u−u/(2π)=4πsinh⁡uu.\begin{aligned} I(u) &=\frac{e^u}{u/(2\pi)} +\frac{e^{-u}}{-u/(2\pi)}\\ &=4\pi\frac{\sinh u}{u}. \end{aligned}

This is the Duistermaat–Heckman specialization of the fixed-point formula Atiyah and Bott 1984, §§6–7. Each fixed-point term has a pole at u=0u=0, but the complete sum does not. The cancellation is a useful check that both the fixed set and the orientations have been handled consistently.

The displayed theorem must be modified in several common situations:

  • if MM is noncompact, a contribution from infinity may survive;
  • if MM has a boundary, Stokes’ theorem produces an explicit boundary term;
  • if MM is not orientable, the pushforward requires the appropriate orientation local system;
  • if the space is singular or an orbifold, one needs a localization theorem for that category, including stabilizer factors;
  • if one specializes the equivariant parameters onto a weight hyperplane, the fixed locus of the chosen subgroup enlarges;
  • if α\alpha is not equivariantly closed, there is no cohomology class to localize.

These are changes to the theorem, not minor numerical corrections.

The structural dictionary is useful:

Finite-dimensional theoremFormal field-theory counterpart
compact manifold MMintegration cycle in field space
Cartan differential dTd_Tsupersymmetry combined with gauge BRST
fixed set MTM^TBPS configurations in every topological sector
normal bundle NFN_Fgauge-fixed transverse fluctuation complex
equivariant Euler classregularized one-loop superdeterminant
tangent orientationmeasure orientation and determinant phase
compactness without boundaryconvergence and vanishing field-space flux

Only the left column is covered by the theorem above. In QFT, field space is infinite dimensional and generally noncompact; the quotient by gauge transformations can be singular; reducible saddles have stabilizers; the Euler class becomes an infinite product; and the contour may be a middle-dimensional cycle in a complexified space. Gauge fixing, zero modes, phases, regulators, anomalies, and contour ends are extra data.

There is a rigorous finite-dimensional supermanifold analogue. Schwarz and Zaboronsky assume a compact supermanifold, a volume-preserving odd vector field, and a compact bosonic square; their localization theorem then concentrates a QQ-invariant integral near the zero set Schwarz and Zaboronsky 1997, §3, Theorem 1. Those hypotheses are informative precisely because an ordinary continuum QFT path integral has not automatically satisfied them. Finite-dimensional localization supplies the architecture for the next page, not a universal proof of it.

Dividing by a zero weight. A zero normal weight signals a nongeneric equivariant parameter or an incorrectly chosen fixed component. Recompute the fixed set before writing an Euler denominator.

Dropping a positive-dimensional fixed component. The numerator and inverse Euler class must still be integrated over that component, including its zero modes.

Calling the QFT column a theorem. Every entry in that column requires a model-specific definition and analytic justification.

1. Nilpotence on invariants. Verify dT2=−uaLVad_T^2=-u^a\mathcal L_{V_a}.

Solution

Using d2=0d^2=0, ιVaιVb+ιVbιVa=0\iota_{V_a}\iota_{V_b}+\iota_{V_b}\iota_{V_a}=0, and Cartan’s identity dιVa+ιVad=LVad\iota_{V_a}+\iota_{V_a}d=\mathcal L_{V_a},

dT2=−ua(dιVa+ιVad)+uaubιVaιVb=−uaLVa.d_T^2 =-u^a\bigl(d\iota_{V_a}+\iota_{V_a}d\bigr) +u^au^b\iota_{V_a}\iota_{V_b} =-u^a\mathcal L_{V_a}.

The last term vanishes because uaubu^au^b is symmetric while the contractions anticommute. Hence dT2=0d_T^2=0 on TT-invariant forms.

2. The ordinary-area limit. Show that the fixed-point answer for S2S^2 has a finite u→0u\to0 limit.

Solution

Expanding sinh⁡u=u+u3/6+⋯\sinh u=u+u^3/6+\cdots gives

I(u)=4π(1+u26+⋯ ),I(u)=4\pi\left(1+\frac{u^2}{6}+\cdots\right),

so I(0)=4π=∫S2ωI(0)=4\pi=\int_{S^2}\omega. The separate 1/u1/u poles cancel only after adding both fixed points.

3. A special equivariant parameter. Suppose a T2T^2 normal representation has weights w1(u1,u2)=u1w_1(u_1,u_2)=u_1 and w2(u1,u2)=u1−u2w_2(u_1,u_2)=u_1-u_2. What goes wrong at u1=u2u_1=u_2?

Solution

The second evaluated weight vanishes, so the chosen one-parameter subgroup acts trivially in that normal direction. Its fixed set is therefore larger than the fixed set used in the isolated-point formula. One must localize with respect to the larger fixed component, or keep generic (u1,u2)(u_1,u_2) until the complete fixed-point sum is formed and only then study a regular limit. Simply omitting w2w_2 changes the normal bundle and is incorrect.

The field-theory argument begins with the finite-parameter Ward identity for a QQ-exact path-integral deformation.

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