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ConceptDescription
Smooth manifoldHausdorff, second countable, locally Euclidean space
Tangent space TpMT_p MSpace of directional derivatives at pp
Vector fieldSmooth section of TMTM
Lie bracket [X,Y][X, Y]Measures non-commutativity of flows
Differential formAlternating covariant tensor field
Exterior derivative ddd2=0d^2 = 0, generalizes gradient/curl/div
Stokes’ theoremMω=Mdω\int_{\partial M} \omega = \int_M d\omega
Riemannian metricSmooth family of inner products on tangent spaces
Levi-Civita connectionUnique torsion-free, metric-compatible connection
GeodesicCurve with zero acceleration γ˙γ˙=0\nabla_{\dot\gamma}\dot\gamma = 0
Riemann curvature tensorMeasures non-commutativity of parallel transport
Gauss-Bonnet theoremTotal curvature = 2πχ(M)2\pi \chi(M) for compact surfaces
  1. Existence and uniqueness of integral curves: For every smooth vector field XX on MM and every pMp \in M, there exists a unique maximal integral curve through pp.

  2. Levi-Civita Theorem: On a Riemannian manifold, there exists a unique metric-compatible, torsion-free connection.

  3. Stokes’ Theorem: For a compact oriented nn-manifold MM with boundary and an (n1)(n-1)-form ω\omega on MM: Mω=Mdω\int_{\partial M} \omega = \int_M d\omega.

  4. Gauss-Bonnet Theorem: For a compact oriented Riemannian 2-manifold: MKdA=2πχ(M)\int_M K\, dA = 2\pi\chi(M).

  5. Frobenius Theorem: A distribution DTM\mathcal{D} \subseteq TM is integrable if and only if it is involutive: [X,Y]Γ(D)[X, Y] \in \Gamma(\mathcal{D}) for all X,YΓ(D)X, Y \in \Gamma(\mathcal{D}).

Christoffel symbols: Γijk=12gk(igj+jgigij)\Gamma^k_{ij} = \frac{1}{2}g^{k\ell}(\partial_i g_{j\ell} + \partial_j g_{i\ell} - \partial_\ell g_{ij})

Geodesic equation: γ¨k+Γijkγ˙iγ˙j=0\ddot\gamma^k + \Gamma^k_{ij}\dot\gamma^i\dot\gamma^j = 0

Riemann curvature tensor: Rijk=iΓjkjΓik+ΓjkmΓimΓikmΓjmR^\ell_{ijk} = \partial_i\Gamma^\ell_{jk} - \partial_j\Gamma^\ell_{ik} + \Gamma^m_{jk}\Gamma^\ell_{im} - \Gamma^m_{ik}\Gamma^\ell_{jm}

Lie bracket (coordinates): [X,Y]=(XjYixjYjXixj)xi[X, Y] = \left(X^j\frac{\partial Y^i}{\partial x^j} - Y^j\frac{\partial X^i}{\partial x^j}\right)\frac{\partial}{\partial x^i}

Exterior derivative: dω=d(1k!ωi1ikdxi1dxik)=1k!ωi1ikxjdxjdxi1dxikd\omega = d\left(\frac{1}{k!}\omega_{i_1\ldots i_k} dx^{i_1} \wedge \cdots \wedge dx^{i_k}\right) = \frac{1}{k!}\frac{\partial\omega_{i_1\ldots i_k}}{\partial x^j} dx^j \wedge dx^{i_1} \wedge \cdots \wedge dx^{i_k}

Lie derivative: LXY=[X,Y],LXf=X(f),LXω=ddtt=0(Φtω)\mathcal{L}_X Y = [X, Y], \quad \mathcal{L}_X f = X(f), \quad \mathcal{L}_X \omega = \frac{d}{dt}\big|_{t=0} (\Phi_t^*\omega)

The following diagram shows how the core concepts of differential geometry relate:

  • Manifold smooth structure\xrightarrow{\text{smooth structure}} Tangent bundle section\xrightarrow{\text{section}} Vector field
  • Vector field integral curve\xrightarrow{\text{integral curve}} Flow Lie bracket\xrightarrow{\text{Lie bracket}} Lie algebra
  • Metric Levi-Civita\xrightarrow{\text{Levi-Civita}} Connection parallel transport\xrightarrow{\text{parallel transport}} Curvature
  • Curvature trace\xrightarrow{\text{trace}} Ricci trace\xrightarrow{\text{trace}} Scalar curvature
  • Connection geodesic equation\xrightarrow{\text{geodesic equation}} Geodesic exponential map\xrightarrow{\text{exponential map}} Normal coordinates
  • Manifold cotangent bundle\xrightarrow{\text{cotangent bundle}} Differential forms exterior derivative\xrightarrow{\text{exterior derivative}} de Rham cohomology

Every compact, connected, oriented 2-manifold is homeomorphic to a sphere with gg handles, where gg is the genus. The Euler characteristic is χ=22g\chi = 2 - 2g.

SurfaceGenus ggEuler characteristic χ\chiTotal curvature
Sphere S2S^2024π4\pi
Torus T2T^2100
Double torus22-24π-4\pi
gg-holed torusgg22g2 - 2g4π(1g)4\pi(1-g)
OperatorAction on ff / ω\omegaIn coordinates
Gradient f\nabla fVector field dual to dfdf(f)i=gijjf(\nabla f)^i = g^{ij}\partial_j f
Divergence X\nabla \cdot XLXdV=(X)dV\mathcal{L}_X dV = (\nabla \cdot X) dV$\nabla \cdot X = \frac{1}{\sqrt{
Laplacian Δf\Delta ff\nabla \cdot \nabla f$\Delta f = \frac{1}{\sqrt{
Curl (×X)(\nabla \times X)(dX)(\star dX^\flat)^\sharpDepends on dimension; in R3\mathbb{R}^3, (×X)i=ϵijkjXk(\nabla \times X)^i = \epsilon^{ijk}\partial_j X_k
  1. Cartan’s magic formula: LXω=d(iXω)+iX(dω)\mathcal{L}_X \omega = d(i_X \omega) + i_X(d\omega).
  2. Poincaré lemma: If dω=0d\omega = 0 (closed form) and the domain is contractible, then ω=dη\omega = d\eta (exact form).
  3. Hodge star: :Ωk(M)Ωnk(M)\star : \Omega^k(M) \to \Omega^{n-k}(M) satisfies =(1)k(nk)\star\star = (-1)^{k(n-k)}.
  4. Kodaira vanishing: On a Kähler manifold with positive line bundle, certain cohomology groups vanish, giving restrictions on the topology.
  1. The Levi-Civita connection depends on the metric, not just the smooth structure. Two metrics on the same smooth manifold generally give different connections, geodesics, and curvatures.

  2. Not every smooth distribution is integrable. The Frobenius theorem gives necessary and sufficient conditions; involutivity ([X,Y]D[X, Y] \in \mathcal{D} for all X,YDX, Y \in \mathcal{D}) must be checked.

  3. The Lie bracket is not the commutator of flows. [X,Y]=0[X, Y] = 0 means flows commute, but [X,Y]0[X, Y] \neq 0 does not mean they do not flow at all — only that the composition order matters.

  4. Stokes’ theorem requires compact support or compact manifold with boundary. For non-compact manifolds, additional decay conditions are needed for the integral to be well-defined.

  5. The exponential map is not globally defined. It is only defined on a neighborhood of zero in TpMT_p M, unless the manifold is geodesically complete (Hopf-Rinow theorem).

  1. Show that S2S^2 and S1×S1S^1 \times S^1 (the torus) are not homeomorphic by comparing their Euler characteristics. Compute χ(S2)\chi(S^2) and χ(T2)\chi(T^2) explicitly using a triangulation.

  2. Prove that the Lie bracket satisfies the Jacobi identity: [X,[Y,Z]]+[Y,[Z,X]]+[Z,[X,Y]]=0[X, [Y, Z]] + [Y, [Z, X]] + [Z, [X, Y]] = 0.

  3. Compute the Christoffel symbols for the sphere S2S^2 with the round metric g=dθ2+sin2θdϕ2g = d\theta^2 + \sin^2\theta\,d\phi^2. Then derive the geodesic equations and verify that great circles are geodesics.

  4. For the 2-torus T2=R2/Z2T^2 = \mathbb{R}^2/\mathbb{Z}^2 with the flat metric inherited from R2\mathbb{R}^2, compute the Riemann curvature tensor. Show that it vanishes identically.

  5. Let MM be a compact oriented Riemannian 2-manifold with χ(M)=0\chi(M) = 0. Use the Gauss-Bonnet theorem to prove that MKdA=0\int_M K\,dA = 0. Give an example of such a manifold.

  6. Show that the exterior derivative dd satisfies d2=0d^2 = 0. Use this to prove that every exact form is closed. Give a counterexample to the converse on a non-contractible manifold.

  7. Compute the de Rham cohomology groups HdR1(S1)H^1_{\text{dR}}(S^1) and HdR1(T2)H^1_{\text{dR}}(T^2). What do they tell you about the topology of these manifolds?

ApplicationManifoldKey Result
General relativitySpacetime (M,g)(M,g)Einstein equations: Rμν12Rgμν=8πGTμνR_{\mu\nu} - \frac{1}{2}Rg_{\mu\nu} = 8\pi G T_{\mu\nu}
Gauge theoryPrincipal bundle PMP \to MYang-Mills equations: dAFA=0d_A \star F_A = 0
String theoryCalabi-Yau 3-foldRicci-flat Kähler metric moduli
Computer visionShape spaceGeodesic distances for shape matching
RoboticsConfiguration space CCMotion planning via geodesics in CC