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Integration on Manifolds

Integration on manifolds is the coordinate-independent integration of differential forms over oriented domains. A kk-form is integrated over a kk-dimensional oriented curve, surface, or manifold:

∫Σω,deg⁡ω=dim⁡Σ.\int_\Sigma \omega, \qquad \deg\omega=\dim\Sigma.

The key mechanism is pullback. A parametrization of the domain pulls the form back to an ordinary form on a region of Euclidean space, where the integral becomes a familiar multiple integral with the correct Jacobian and orientation signs already built in.

Helpful background. Review Differential Forms for wedge products and Exterior Derivative for the derivative in Stokes’ theorem.

A Berry connection is integrated along a path, while its curvature is integrated over a surface. To calculate either integral, substitute a parametrization into the form. This operation, called pullback, supplies the familiar Jacobian factors and the orientation signs.

Let ω\omega be a kk-form on a manifold MM, and let

Φ:D→M\Phi:D\to M

parametrize a kk-dimensional domain Σ⊂M\Sigma\subset M, where D⊂RkD\subset\mathbb R^k. The integral is defined by

∫Σω=∫DΦ∗ω.\int_\Sigma \omega = \int_D \Phi^*\omega.

Here Φ∗ω\Phi^*\omega is the pullback of the form to the parameter domain. It inserts the tangent vectors produced by the parametrization and automatically supplies the Jacobian factors.

This is why the coordinate formulas in Differential Forms look determinant-like: the determinant is the form’s response to oriented tangent directions.

Let

α=αi(x) dxi\alpha=\alpha_i(x)\,dx^i

be a 1-form, and let

γ:[a,b]→M,t↦x(t),\gamma:[a,b]\to M, \qquad t\mapsto x(t),

be an oriented curve. Pulling back α\alpha gives

γ∗α=αi(x(t))x˙i(t) dt.\gamma^*\alpha = \alpha_i(x(t))\dot x^i(t)\,dt.

Therefore

∫γα=∫abαi(x(t))x˙i(t) dt.\int_\gamma \alpha = \int_a^b \alpha_i(x(t))\dot x^i(t)\,dt.

Reversing the curve orientation changes the sign. If γˉ(t)=γ(a+b−t)\bar\gamma(t)=\gamma(a+b-t) is the reversed path, then

∫γˉα=−∫γα.\int_{\bar\gamma}\alpha = - \int_\gamma\alpha.

This is the line-integral structure behind Berry phases and circulation integrals.

Let

ω=∑i<jωij(x) dxi∧dxj\omega = \sum_{i<j} \omega_{ij}(x)\,dx^i\wedge dx^j

be a 2-form, and let

Φ:D→M,(u,v)↦x(u,v),\Phi:D\to M, \qquad (u,v)\mapsto x(u,v),

parametrize an oriented surface. Then

Φ∗ω=∑i<jωij(x(u,v))(∂xi∂u∂xj∂v−∂xi∂v∂xj∂u)du∧dv.\Phi^*\omega = \sum_{i<j} \omega_{ij}(x(u,v)) \left( \frac{\partial x^i}{\partial u} \frac{\partial x^j}{\partial v} - \frac{\partial x^i}{\partial v} \frac{\partial x^j}{\partial u} \right) du\wedge dv.

Thus

∫Σω=∫DΦ∗ω.\int_\Sigma\omega = \int_D \Phi^*\omega.

Changing the order of the parameters from (u,v)(u,v) to (v,u)(v,u) reverses the orientation and changes the sign.

An orientation is a consistent choice of positive ordered tangent bases. In two dimensions, saying that (∂u,∂v)(\partial_u,\partial_v) is positive is the same kind of choice as saying that du∧dvdu\wedge dv is the positive area form on the parameter domain.

The sign of a form integral depends on this choice:

∫−Σω=−∫Σω,\int_{-\Sigma}\omega = - \int_\Sigma\omega,

where −Σ-\Sigma denotes the same domain with the opposite orientation.

For curves, orientation is the direction of traversal. For surfaces, orientation is a choice of which ordered tangent-pair direction is positive. In embedded Euclidean three-space, this is often represented by a normal vector using the right-hand rule, but the form definition does not require an ambient normal.

Stokes theorem requires a convention for orienting the boundary ∂Σ\partial\Sigma. The standard convention is:

An ordered basis of T(∂Σ)T(\partial\Sigma) is positive when the outward normal followed by that basis gives the orientation of Σ\Sigma.

For an interval [a,b][a,b] with its usual orientation, the boundary orientation is

∂[a,b]={b}−{a}.\partial[a,b]=\{b\}-\{a\}.

For an oriented region in the plane with the usual dx∧dydx\wedge dy orientation, the outer boundary is counterclockwise and any boundary around a hole is clockwise. In either case, the region stays on the left as one traverses its boundary. The annulus example illustrates why both boundary components matter.

This sign convention is what makes the fundamental theorem of calculus and Green’s theorem appear with the usual signs.

On an nn-dimensional oriented manifold, an nn-form can be integrated over nn-dimensional regions. In local coordinates,

Ω=f(x) dx1∧⋯∧dxn\Omega = f(x)\,dx^1\wedge\cdots\wedge dx^n

integrates as

∫UΩ=∫φ(U)f(x) dx1⋯dxn\int_U \Omega = \int_{\varphi(U)} f(x)\,dx^1\cdots dx^n

in an orientation-preserving chart.

A scalar function by itself is not automatically integrable over a manifold in a coordinate-independent way. To integrate a scalar ff, one needs a chosen volume form or measure, such as the metric volume form on a Riemannian manifold:

∫Mf dVg.\int_M f\,dV_g.

This distinction prevents a common confusion: forms are integrands; scalar functions become integrands only after choosing the measure or volume form.

The standard area 2-form on the plane is

dx∧dy.dx\wedge dy.

Use polar coordinates

x=rcos⁡θ,y=rsin⁡θ.x=r\cos\theta, \qquad y=r\sin\theta.

Then

dx=cos⁡θ dr−rsin⁡θ dθ,dy=sin⁡θ dr+rcos⁡θ dθ.\begin{aligned} dx&=\cos\theta\,dr-r\sin\theta\,d\theta,\\ dy&=\sin\theta\,dr+r\cos\theta\,d\theta. \end{aligned}

Therefore

dx∧dy=r dr∧dθ.dx\wedge dy = r\,dr\wedge d\theta.

The familiar polar-coordinate Jacobian appears because the 2-form has been pulled back:

∫diskdx∧dy=∫02π∫0Rr dr dθ=πR2.\int_{\text{disk}} dx\wedge dy = \int_0^{2\pi}\int_0^R r\,dr\,d\theta = \pi R^2.

No separate mnemonic for the Jacobian is needed; it is the coefficient of the pulled-back form.

Let Σ\Sigma be a compact oriented kk-dimensional manifold with boundary, and let ω\omega be a smooth (k−1)(k-1)-form on a neighborhood of Σ\Sigma. Stokes theorem says

∫Σdω=∫∂Σω.\int_\Sigma d\omega = \int_{\partial\Sigma}\omega.

The left side integrates a kk-form over the kk-dimensional region. The right side integrates a (k−1)(k-1)-form over the oriented boundary.

This is the master theorem behind several familiar results:

  • the fundamental theorem of calculus;
  • Green’s theorem in the plane;
  • the Kelvin-Stokes curl theorem;
  • the divergence theorem.

The power of the form statement is that the same equation works in any dimension and any coordinate system where the hypotheses are satisfied.

Let ff be a smooth function on an interval [a,b][a,b]. Since

df=f′(x) dx,df=f'(x)\,dx,

Stokes theorem gives

∫[a,b]df=∫∂[a,b]f.\int_{[a,b]}df = \int_{\partial[a,b]}f.

Using the boundary orientation ∂[a,b]={b}−{a}\partial[a,b]=\{b\}-\{a\},

∫abf′(x) dx=f(b)−f(a).\int_a^b f'(x)\,dx = f(b)-f(a).

Thus the fundamental theorem of calculus is the one-dimensional case of Stokes theorem.

Let

α=P(x,y) dx+Q(x,y) dy\alpha=P(x,y)\,dx+Q(x,y)\,dy

on a region DD in the plane. Then

dα=(∂Q∂x−∂P∂y)dx∧dy.d\alpha = \left( \frac{\partial Q}{\partial x} - \frac{\partial P}{\partial y} \right) dx\wedge dy.

Stokes theorem gives

∫D(∂Q∂x−∂P∂y)dx∧dy=∫∂DP dx+Q dy.\int_D \left( \frac{\partial Q}{\partial x} - \frac{\partial P}{\partial y} \right) dx\wedge dy = \int_{\partial D} P\,dx+Q\,dy.

This is Green’s theorem. The three-dimensional curl theorem is the same statement with a 1-form integrated around the boundary of an oriented surface.

In Euclidean three-space, represent a vector field B=(Bx,By,Bz)\mathbf B=(B_x,B_y,B_z) by the flux 2-form

B=Bx dy∧dz+By dz∧dx+Bz dx∧dy.\mathcal B = B_x\,dy\wedge dz + B_y\,dz\wedge dx + B_z\,dx\wedge dy.

Then

dB=(∇⋅B) dx∧dy∧dz.d\mathcal B = (\nabla\cdot\mathbf B)\,dx\wedge dy\wedge dz.

Stokes theorem gives

∫VdB=∫∂VB,\int_V d\mathcal B = \int_{\partial V}\mathcal B,

which is the divergence theorem after translating the 2-form flux back into vector notation.

For a Berry connection one-form AnA_n in a smooth eigenvector frame that is periodic around a closed loop CC, the Berry phase is, modulo 2π2\pi,

γn[C]=∮CAn.\gamma_n[C] = \oint_C A_n.

For a nonperiodic frame, include the endpoint overlap. If C=∂ΣC=\partial\Sigma and a smooth gauge is available on the surface Σ\Sigma, Stokes theorem gives

∮CAn=∫ΣdAn=∫ΣFn.\oint_C A_n = \int_\Sigma dA_n = \int_\Sigma F_n.

This is the geometric form of the statement that Berry phase can be computed as curvature flux through a spanning surface.

The hypotheses matter. If no single smooth gauge is available on Σ\Sigma, or if the surface crosses a degeneracy where the eigenstate is not defined, one must use patches or remove singular points. The physical discussion is in Berry Phase, while the connection and curvature objects are defined in Connections and Curvature; this page explains the integration theorem.

If a domain is not covered by one coordinate chart, integration is defined by covering it with charts, using a partition of unity, integrating in each chart, and summing the results. The coordinate changes agree because differential forms transform with the correct Jacobian factors.

For most quantum-mechanics calculations, the practical lesson is simpler: when a single chart has a coordinate singularity, do not automatically conclude that the integral or form is singular. Check whether the form is globally defined, whether patches are needed, and whether the singular point is actually part of the manifold.

  • Integrating a kk-form over a domain of the wrong dimension.
  • Ignoring orientation and losing a sign.
  • Treating du dvdu\,dv as coordinate-independent without pulling back a form.
  • Forgetting that a scalar function needs a volume form or measure before it can be integrated invariantly.
  • Applying Stokes theorem when the form is not smooth on the region.
  • Using a single gauge or chart across a surface where it is not defined.
  • Forgetting the induced boundary orientation.
  • Confusing a coordinate singularity with a genuine singularity of the integrand.
  1. Use Stokes theorem to compute ∫Cx dy−y dx\int_C x\,dy-y\,dx for the counterclockwise unit circle.
Solution

Let

α=x dy−y dx.\alpha=x\,dy-y\,dx.

Then

dα=2 dx∧dy.d\alpha = 2\,dx\wedge dy.

If DD is the unit disk and C=∂DC=\partial D with counterclockwise orientation, Stokes theorem gives

∫Cα=∫Ddα=∫D2 dx∧dy=2π.\int_C\alpha = \int_D d\alpha = \int_D 2\,dx\wedge dy = 2\pi.
  1. Let f(x)=x3f(x)=x^3 on [0,2][0,2]. Verify the one-dimensional Stokes theorem.
Solution

The exterior derivative is

df=3x2 dx.df=3x^2\,dx.

Thus

∫[0,2]df=∫023x2 dx=8.\int_{[0,2]}df = \int_0^2 3x^2\,dx = 8.

The boundary orientation is ∂[0,2]={2}−{0}\partial[0,2]=\{2\}-\{0\}, so

∫∂[0,2]f=f(2)−f(0)=8.\int_{\partial[0,2]}f = f(2)-f(0) = 8.
  1. Derive the polar-coordinate area element by pulling back dx∧dydx\wedge dy.
Solution

For x=rcos⁡θx=r\cos\theta and y=rsin⁡θy=r\sin\theta,

dx=cos⁡θ dr−rsin⁡θ dθ,dy=sin⁡θ dr+rcos⁡θ dθ.dx=\cos\theta\,dr-r\sin\theta\,d\theta, \qquad dy=\sin\theta\,dr+r\cos\theta\,d\theta.

Wedge them:

dx∧dy=(cos⁡θ dr−rsin⁡θ dθ)∧(sin⁡θ dr+rcos⁡θ dθ)=r(cos⁡2θ+sin⁡2θ) dr∧dθ=r dr∧dθ.\begin{aligned} dx\wedge dy &= (\cos\theta\,dr-r\sin\theta\,d\theta) \wedge (\sin\theta\,dr+r\cos\theta\,d\theta)\\ &= r(\cos^2\theta+\sin^2\theta)\,dr\wedge d\theta\\ &= r\,dr\wedge d\theta. \end{aligned}
  1. Let R=[0,Lx]×[0,Ly]R=[0,L_x]\times[0,L_y] with the standard orientation. Compute ∫∂Rx dy\int_{\partial R}x\,dy.
Solution

Let α=x dy\alpha=x\,dy. Then

dα=dx∧dy.d\alpha=dx\wedge dy.

By Stokes theorem,

∫∂Rx dy=∫Rdx∧dy=LxLy.\int_{\partial R}x\,dy = \int_R dx\wedge dy = L_xL_y.
  1. Suppose F=F0 dR1∧dR2F=F_0\,dR^1\wedge dR^2 is a constant Berry-curvature 2-form on a rectangular patch 0≤R1≤a0\le R^1\le a, 0≤R2≤b0\le R^2\le b. If AA is a smooth connection on the patch with dA=FdA=F, what is ∮∂ΣA\oint_{\partial\Sigma}A?
Solution

By Stokes theorem,

∮∂ΣA=∫ΣdA=∫ΣF.\oint_{\partial\Sigma}A = \int_\Sigma dA = \int_\Sigma F.

Since FF is constant,

∫ΣF=F0ab.\int_\Sigma F = F_0ab.
  1. Why can Stokes theorem not be applied blindly across a singular gauge patch?
Solution

Stokes theorem assumes the form is smooth on the region being integrated. If a gauge potential is not defined or not smooth somewhere on the spanning surface, the hypothesis fails. One must use multiple patches, remove the singular point and account for the new boundary, or reformulate the calculation in terms of globally defined objects.

  • T. Frankel, The Geometry of Physics, 3rd ed., Cambridge University Press, 2011.
  • J. M. Lee, Introduction to Smooth Manifolds, 2nd ed., Springer, 2013.
  • L. W. Tu, An Introduction to Manifolds, 2nd ed., Springer, 2011.