Book 9A

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Course 9Book 9A: Metrics, Connections and CurvatureChapter 6

The Laplacian and the Bochner Formula

Calculus on Riemannian manifolds, spherical harmonics and commuting derivatives.

28 min read · Updated Oct 3, 2026

Read with Lee, Introduction to Riemannian Manifolds (2nd edition), chapter 2 (the gradient, divergence and Laplacian, the divergence theorem) and chapter 7 (the Ricci identities for commuting covariant derivatives). Petersen's Riemannian Geometry, chapters 2–3 and the Bochner technique chapter, is the second voice.

In this chapter · 8 sections
  1. 6.1The Earth's gravity in spherical harmonics
  2. 6.2Gradient, divergence, Hessian and Laplacian
  3. 6.3Eigenvalues: spheres and tori
  4. 6.4Commuting derivatives
  5. 6.5The Bochner formula
  6. 6.6Laplacians on tensors
  7. 6.7History
  8. 6.8Exercises

The Ricci flow is a heat equation, and a heat equation needs a Laplacian. This chapter builds calculus on a Riemannian manifold: gradient, divergence, Hessian and the Laplace–Beltrami operator, integration by parts on closed manifolds, and the eigenvalues of the Laplacian on spheres and tori. It then does the one computation every evolution equation of the Ricci flow depends on: commuting covariant derivatives, where curvature appears as the price of changing the order of differentiation. The first and most famous result of that kind is the Bochner formula, which turns a lower bound on Ricci curvature into control of harmonic and eigen-functions. Its first application, Lichnerowicz's eigenvalue estimate, says that positive Ricci curvature makes a manifold "ring" at a high pitch.

By the end of this chapter you will be able to:

  • compute gradients, divergences, Hessians and Laplacians in coordinates and in warped products;
  • integrate by parts on a closed Riemannian manifold, and state Green's identities;
  • describe the eigenvalues and eigenfunctions of the Laplacian on spheres and flat tori;
  • commute covariant derivatives of vector fields, 1-forms and 2-tensors;
  • prove the Bochner formula and Lichnerowicz's estimate, and define the Lichnerowicz Laplacian.

The Earth's gravity in spherical harmonics

In the world Data EGM2008

Outside the Earth, the gravitational potential VV is harmonic, ΔV=0\Delta V = 0, so on each sphere around the Earth's centre it can be expanded in spherical harmonics, the eigenfunctions of the Laplacian on the sphere. Geodesists describe the Earth's gravity field by the coefficients of that expansion. The Earth Gravitational Model 2008 (EGM2008, Pavlis and colleagues, Journal of Geophysical Research, 2012), built from satellite data (including GRACE, 9A.4 Curvature and What It Means) and from gravity measured on land, at sea and from the air, goes up to degree 21592159, resolving features about 1010 km across.

The low degrees have plain physical meanings. Degree 00 is the total mass. Degree 11 vanishes when the origin is the centre of mass. The largest correction is the degree-22 zonal term, with coefficient J2≈1.083×10−3J_2 \approx 1.083\times10^{-3}, which describes the Earth's equatorial bulge, the flattening of 9A.1 Riemannian Metrics and Model Spaces. It is the term that makes the orbits of satellites precess, which is what lets sun-synchronous satellites keep the same local time of day as they pass overhead.

Gradient, divergence, Hessian and Laplacian

On (M,g)(M, g):

  • the gradient of a function is the vector field dual to dfdf: ⟨∇f,X⟩=Xf\langle\nabla f, X\rangle = Xf, or ∇if=gij∂jf\nabla^if = g^{ij}\partial_jf;
  • the divergence of a vector field is the trace of its covariant derivative: div⁡X=∇iXi\operatorname{div}X = \nabla_iX^i;
  • the Hessian is ∇2f=∇df\nabla^2f = \nabla df, with components ∇i∇jf=∂i∂jf−Γijk∂kf\nabla_i\nabla_jf = \partial_i\partial_jf - \Gamma_{ij}^k\partial_kf, symmetric (9A.2 Connections);
  • the Laplacian (Laplace–Beltrami operator) is Δf=div⁡∇f=gij∇i∇jf\Delta f = \operatorname{div}\nabla f = g^{ij}\nabla_i\nabla_jf, the trace of the Hessian.

In coordinates, with ∣g∣=det⁡(gij)|g| = \det(g_{ij}),

div⁡X=1∣g∣∂i(∣g∣Xi),Δf=1∣g∣∂i(∣g∣ gij∂jf)\operatorname{div}X = \frac{1}{\sqrt{|g|}}\partial_i\big(\sqrt{|g|}X^i\big), \qquad \Delta f = \frac{1}{\sqrt{|g|}}\partial_i\Big(\sqrt{|g|}\,g^{ij}\partial_jf\Big)

(Exercise 6.3). The sign convention is the analyst's: on Rn\mathbb{R}^n, Δ=∑∂i2\Delta = \sum\partial_i^2, and −Δ-\Delta has nonnegative eigenvalues (8A.7 Tensors and Index Notation). For a warped product dr2+φ(r)2gSn−1dr^2 + \varphi(r)^2g_{S^{n-1}},

Δf=∂r2f+(n−1)φ′φ∂rf+1φ2ΔSn−1f,\Delta f = \partial_r^2f + (n - 1)\frac{\varphi'}{\varphi}\partial_rf + \frac{1}{\varphi^2}\Delta_{S^{n-1}}f,

where (n−1)φ′φ(n - 1)\frac{\varphi'}{\varphi} is the mean curvature of the sphere {r=const}\{r = \text{const}\}. On Rn\mathbb{R}^n it is n−1r\frac{n - 1}{r}, giving the familiar radial Laplacian f′′+n−1rf′f'' + \frac{n - 1}{r}f' of 6A.2 Harmonic Functions.

Integration by parts. On a closed (compact, boundaryless) manifold the divergence theorem (8A.8 Differential Forms and Stokes’ Theorem) gives ∫Mdiv⁡X dV=0\int_M\operatorname{div}X\,dV = 0. Applied to X=f∇hX = f\nabla h:

∫MfΔh dV=−∫M⟨∇f,∇h⟩ dV=∫MhΔf dV.\int_Mf\Delta h\,dV = -\int_M\langle\nabla f, \nabla h\rangle\,dV = \int_Mh\Delta f\,dV.

So Δ\Delta is symmetric and −Δ-\Delta is nonnegative: if Δf=−λf\Delta f = -\lambda f, then λ∫f2=∫∣∇f∣2≥0\lambda\int f^2 = \int|\nabla f|^2 \geq 0, with λ=0\lambda = 0 only for constants (on a connected MM). The maximum principle of 6A.4 Maximum Principles carries over word for word: at an interior maximum of ff, ∇f=0\nabla f = 0 and ∇2f≤0\nabla^2f \leq 0, so Δf≤0\Delta f \leq 0. These are the two tools, integration and the maximum principle, of every estimate in the Ricci flow.

Eigenvalues: spheres and tori

The Laplacian of a closed manifold has eigenvalues 0=λ0<λ1≤λ2≤⋯→∞0 = \lambda_0 < \lambda_1 \leq \lambda_2 \leq \dots \to \infty (of −Δ-\Delta), with smooth eigenfunctions forming an orthonormal basis of L2L^2 (the spectral theorem for compact self-adjoint operators, 4A.7 Compact Operators and Spectra). The first nonzero eigenvalue λ1\lambda_1 is the decay rate of the heat equation towards its average, and the square of the lowest pitch of a drum shaped like the manifold. Two cases can be computed completely.

Flat tori. On Rn/Λ\mathbb{R}^n/\Lambda, the eigenfunctions are e2πi⟨ξ,x⟩e^{2\pi i\langle\xi, x\rangle} for ξ\xi in the dual lattice Λ∗\Lambda^*, with eigenvalues 4π2∣ξ∣24\pi^2|\xi|^2: Fourier series (2B.7 Fourier Series and the First Heat Equation) again.

Spheres. On the unit SnS^n, the eigenvalues of −Δ-\Delta are

λk=k(k+n−1),k=0,1,2,…,\lambda_k = k(k + n - 1), \qquad k = 0, 1, 2, \dots,

and the eigenfunctions with eigenvalue λk\lambda_k are the restrictions to SnS^n of the homogeneous harmonic polynomials of degree kk on Rn+1\mathbb{R}^{n + 1}, the spherical harmonics of degree kk (Exercise 6.5). On S2S^2, λk=k(k+1)\lambda_k = k(k + 1) with multiplicity 2k+12k + 1: the functions YkmY_k^m, ∣m∣≤k|m| \leq k, of quantum mechanics, chemistry and geodesy (Figure 6.1). The first nonzero eigenvalue of the unit SnS^n is λ1=n\lambda_1 = n, with eigenfunctions the coordinate functions x1,…,xn+1x_1, \dots, x_{n + 1}.

Figure 6.1. Nodal lines (where the function vanishes) of the real spherical harmonics Pkm(cos⁡θ)cos⁡mϕP_k^m(\cos\theta)\cos m\phi on S2S^2, for degree k≤3k \leq 3 and order 0≤m≤k0 \leq m \leq k, computed from the roots of the associated Legendre functions. Each has k−mk - m circles of latitude and mm great circles through the poles: kk nodal circles in all, for eigenvalue k(k+1)k(k + 1).
In the world Data The cosmic microwave background

The temperature of the cosmic microwave background, the radiation left from about 380,000380{,}000 years after the Big Bang, is a function on the sphere of directions in the sky, uniform to about one part in 100,000100{,}000. Cosmologists expand its fluctuations in spherical harmonics and plot the angular power spectrum, the average squared coefficient at each degree ℓ\ell. Its peaks, the first near ℓ≈220\ell \approx 220, an angular scale of about a degree, record sound waves in the early plasma, and their positions and heights measured by the WMAP and Planck satellites determine the geometry and composition of the universe. Among other things, the first peak's position is the main evidence that space on large scales is close to flat.

Commuting derivatives

Second covariant derivatives of functions commute (∇i∇jf=∇j∇if\nabla_i\nabla_jf = \nabla_j\nabla_if, because the connection is torsion-free). Second covariant derivatives of tensors do not, and the commutator is curvature. For a vector field, a 1-form and a 2-tensor, the Ricci identities are

∇i∇jXk−∇j∇iXk=RijlkXl,\nabla_i\nabla_jX^k - \nabla_j\nabla_iX^k = R_{ijl}{}^kX^l,
∇i∇jωk−∇j∇iωk=−Rijklωl,\nabla_i\nabla_j\omega_k - \nabla_j\nabla_i\omega_k = -R_{ijk}{}^l\omega_l,
∇i∇jhkl−∇j∇ihkl=−Rijkmhml−Rijlmhkm,\nabla_i\nabla_jh_{kl} - \nabla_j\nabla_ih_{kl} = -R_{ijk}{}^mh_{ml} - R_{ijl}{}^mh_{km},

one curvature term for each index, with ++ for upper and −- for lower indices, like the Christoffel terms of 9A.2 Connections (Lee, chapter 7). The first is the definition of RR applied to XX; the second follows by applying the first to ω(X)\omega(X), a function (Exercise 6.6); the third follows from the second by the product rule.

The most used consequence, the one in the rehearsal exercise of this chapter and in every soliton identity of 11B.1 Ricci Solitons, is the commutation of the Laplacian with the gradient:

Δ∇jf=∇jΔf+Rjk∇kf.\Delta\nabla_jf = \nabla_j\Delta f + R_{jk}\nabla^kf.

Taking the Laplacian of a gradient produces a Ricci term. That term is the bridge between Ricci curvature and analysis.

The Bochner formula

Theorem 6.1 Bochner's formula

For every smooth function ff on a Riemannian manifold,

12Δ∣∇f∣2=∣∇2f∣2+⟨∇f,∇Δf⟩+Ric⁡(∇f,∇f).\tfrac12\Delta|\nabla f|^2 = |\nabla^2f|^2 + \langle\nabla f, \nabla\Delta f\rangle + \operatorname{Ric}(\nabla f, \nabla f).

Proof. Since ∇g=0\nabla g = 0, ∇i∣∇f∣2=2∇i∇jf ∇jf\nabla_i|\nabla f|^2 = 2\nabla_i\nabla_jf\,\nabla^jf, and applying ∇i\nabla^i,

12Δ∣∇f∣2=∇i∇i∇jf ∇jf+∇i∇jf ∇i∇jf.\tfrac12\Delta|\nabla f|^2 = \nabla^i\nabla_i\nabla_jf\,\nabla^jf + \nabla_i\nabla_jf\,\nabla^i\nabla^jf.

The second term is ∣∇2f∣2|\nabla^2f|^2. In the first, ∇i∇i∇jf=Δ∇jf=∇jΔf+Rjk∇kf\nabla^i\nabla_i\nabla_jf = \Delta\nabla_jf = \nabla_j\Delta f + R_{jk}\nabla^kf by the commutation formula above. Contracting with ∇jf\nabla^jf gives ⟨∇f,∇Δf⟩+Ric⁡(∇f,∇f)\langle\nabla f, \nabla\Delta f\rangle + \operatorname{Ric}(\nabla f, \nabla f).

The formula says that for a harmonic function (Δf=0\Delta f = 0), 12Δ∣∇f∣2=∣∇2f∣2+Ric⁡(∇f,∇f)\frac12\Delta|\nabla f|^2 = |\nabla^2f|^2 + \operatorname{Ric}(\nabla f, \nabla f): if Ric⁡≥0\operatorname{Ric} \geq 0, then ∣∇f∣2|\nabla f|^2 is subharmonic. That is the start of the Bochner technique: on a closed manifold with Ric⁡≥0\operatorname{Ric} \geq 0, integrating shows every harmonic 1-form is parallel, so the first Betti number is at most nn (Bochner, 1946). In the Ricci flow the same pattern, "a square plus a curvature term", appears in Hamilton's Harnack inequality (11B.2 Ancient Solutions and the Harnack Inequality), the Li–Yau estimate (9B.7 The Heat Equation on a Manifold) and Perelman's entropy (12A.3 The 𝓦-Entropy).

Theorem 6.2 Lichnerowicz's estimate

If MM is closed and Ric⁡≥(n−1)kg\operatorname{Ric} \geq (n - 1)kg with k>0k > 0, then the first nonzero eigenvalue of −Δ-\Delta satisfies λ1≥nk\lambda_1 \geq nk.

Proof. Let Δf=−λf\Delta f = -\lambda f with λ>0\lambda > 0. Integrate Bochner's formula; the left side integrates to zero:

0=∫∣∇2f∣2−λ∫∣∇f∣2+∫Ric⁡(∇f,∇f).0 = \int|\nabla^2f|^2 - \lambda\int|\nabla f|^2 + \int\operatorname{Ric}(\nabla f, \nabla f).

By the Cauchy–Schwarz inequality for the trace (8A.7 Tensors and Index Notation), ∣∇2f∣2≥1n(Δf)2|\nabla^2f|^2 \geq \frac1n(\Delta f)^2, and ∫(Δf)2=λ2∫f2=λ∫∣∇f∣2\int(\Delta f)^2 = \lambda^2\int f^2 = \lambda\int|\nabla f|^2. So

0≥(λn−λ+(n−1)k)∫∣∇f∣2,0 \geq \Big(\frac\lambda n - \lambda + (n - 1)k\Big)\int|\nabla f|^2,

and since ∫∣∇f∣2>0\int|\nabla f|^2 > 0, n−1nλ≥(n−1)k\frac{n - 1}{n}\lambda \geq (n - 1)k.

The unit sphere has Ric⁡=(n−1)g\operatorname{Ric} = (n - 1)g and λ1=n\lambda_1 = n, so the estimate is sharp, and Morio Obata (1962) proved the sphere is the only case of equality. Ricci curvature bounded below by a positive constant forces a spectral gap, and hence exponentially fast decay of heat: positive curvature makes diffusion efficient.

Laplacians on tensors

The rough Laplacian of a tensor field is ΔT=gij∇i∇jT\Delta T = g^{ij}\nabla_i\nabla_jT, the trace of its second covariant derivative. For a symmetric 2-tensor hh, the Lichnerowicz Laplacian adds curvature terms:

ΔLhjk=Δhjk+2Rpjkqhpq−Rjphpk−Rkphpj\Delta_Lh_{jk} = \Delta h_{jk} + 2R_{pjkq}h^{pq} - R_{jp}h^p{}_k - R_{kp}h^p{}_j

(in this guide's conventions; it is checked on the sphere in Exercise 6.8). It arises from linearising the Ricci tensor, and under the Ricci flow the Ricci tensor itself evolves by

∂tRjk=ΔLRjk=ΔRjk+2RpjkqRpq−2RjpRpk,\partial_tR_{jk} = \Delta_LR_{jk} = \Delta R_{jk} + 2R_{pjkq}R^{pq} - 2R_{jp}R^p{}_k,

derived in 11A.2 How Curvature Evolves. You verify it on the shrinking sphere in Exercise 6.8.

In the world In use The cotangent Laplacian

Computer graphics and geometry processing work with surfaces given as triangle meshes, and they need a Laplacian on them: to smooth noisy scans, to flatten surfaces for texture maps, to compute geodesic distances by the heat method, to deform shapes. The standard choice is the cotangent Laplacian: at a vertex ii,

(Δf)i=12Ai∑j∼i(cot⁡αij+cot⁡βij)(fj−fi),(\Delta f)_i = \frac{1}{2A_i}\sum_{j \sim i}(\cot\alpha_{ij} + \cot\beta_{ij})(f_j - f_i),

where αij\alpha_{ij} and βij\beta_{ij} are the angles opposite the edge ijij in its two triangles and AiA_i is an area assigned to the vertex (Figure 6.2). It is the matrix of linear finite elements for ∫∣∇f∣2\int|\nabla f|^2. Ulrich Pinkall and Konrad Polthier made it the basis of their computation of discrete minimal surfaces (Experimental Mathematics, 1993), and it has been the default discrete Laplace–Beltrami operator in geometry processing since.

Figure 6.2. The cotangent weight of the edge ijij: the two angles αij\alpha_{ij} and βij\beta_{ij} opposite it, in the two triangles that share it. The weight 12(cot⁡αij+cot⁡βij)\frac12(\cot\alpha_{ij} + \cot\beta_{ij}) is positive when αij+βij<π\alpha_{ij} + \beta_{ij} < \pi.
Where this goes Where these identities go

The evolution equations of 11A.2 How Curvature Evolves are long computations made of three moves: vary the Christoffel symbols (the last exercise of 9A.2 Connections), commute covariant derivatives (this chapter), and use the Bianchi identities (9A.4 Curvature and What It Means). The heat equation on a manifold, with its maximum principle and its Li–Yau estimate, is the subject of 9B.7 The Heat Equation on a Manifold; the Bochner formula is its engine.

History

Laplace and Legendre introduced spherical harmonics in the 1780s, studying the gravitational attraction of planets. Eugenio Beltrami defined the Laplacian of a Riemannian metric in the 1860s. Salomon Bochner published his formula and its consequences for Betti numbers in 1946. André Lichnerowicz proved the eigenvalue estimate in 1958 and introduced his Laplacian in his work on Einstein metrics; Obata's rigidity theorem followed in 1962.

Recall Where we stand

The Laplace–Beltrami operator Δf=gij∇i∇jf=1∣g∣∂i(∣g∣gij∂jf)\Delta f = g^{ij}\nabla_i\nabla_jf = \frac{1}{\sqrt{|g|}}\partial_i(\sqrt{|g|}g^{ij}\partial_jf) is symmetric and nonpositive on a closed manifold, satisfies the maximum principle, and on warped products reads f′′+(n−1)φ′φf′+φ−2ΔSff'' + (n - 1)\frac{\varphi'}{\varphi}f' + \varphi^{-2}\Delta_Sf. On the unit SnS^n its eigenvalues are k(k+n−1)k(k + n - 1), with spherical harmonics as eigenfunctions; on flat tori, 4π2∣ξ∣24\pi^2|\xi|^2. Covariant derivatives of tensors commute up to curvature terms, one per index; in particular Δ∇f=∇Δf+Ric⁡(∇f)\Delta\nabla f = \nabla\Delta f + \operatorname{Ric}(\nabla f). Bochner's formula 12Δ∣∇f∣2=∣∇2f∣2+⟨∇f,∇Δf⟩+Ric⁡(∇f,∇f)\frac12\Delta|\nabla f|^2 = |\nabla^2f|^2 + \langle\nabla f, \nabla\Delta f\rangle + \operatorname{Ric}(\nabla f, \nabla f) gives Lichnerowicz's bound λ1≥nk\lambda_1 \geq nk when Ric⁡≥(n−1)k\operatorname{Ric} \geq (n - 1)k. The Ricci tensor evolves under the flow by the Lichnerowicz Laplacian. 9A.7 Jacobi Fields and Curvature versus Topology varies geodesics and turns Ricci curvature into topology.

Exercises

Exercise 6.3 The coordinate formula

Show that Γiki=∂klog⁡∣g∣\Gamma_{ik}^i = \partial_k\log\sqrt{|g|} (use ∂klog⁡det⁡g=gij∂kgij\partial_k\log\det g = g^{ij}\partial_kg_{ij}), and deduce ∇iXi=1∣g∣∂i(∣g∣Xi)\nabla_iX^i = \frac{1}{\sqrt{|g|}}\partial_i(\sqrt{|g|}X^i) and the formula for Δ\Delta. Then derive the warped-product formula for functions of rr alone.

Solution

Γiki=12gil(∂igkl+∂kgil−∂lgik)=12gil∂kgil\Gamma_{ik}^i = \frac12g^{il}(\partial_ig_{kl} + \partial_kg_{il} - \partial_lg_{ik}) = \frac12g^{il}\partial_kg_{il}, the other two terms cancelling by symmetry of gilg^{il}; this is 12∂klog⁡∣g∣\frac12\partial_k\log|g|. So ∇iXi=∂iXi+ΓikiXk=∂iXi+Xk∂klog⁡∣g∣=1∣g∣∂i(∣g∣Xi)\nabla_iX^i = \partial_iX^i + \Gamma_{ik}^iX^k = \partial_iX^i + X^k\partial_k\log\sqrt{|g|} = \frac{1}{\sqrt{|g|}}\partial_i(\sqrt{|g|}X^i). With X=∇fX = \nabla f this gives Δ\Delta. For g=dr2+φ2gSg = dr^2 + \varphi^2g_S, ∣g∣=φn−1∣gS∣\sqrt{|g|} = \varphi^{n - 1}\sqrt{|g_S|}, and for f=f(r)f = f(r), Δf=φ1−n(φn−1f′)′=f′′+(n−1)φ′φf′\Delta f = \varphi^{1 - n}(\varphi^{n - 1}f')' = f'' + (n - 1)\frac{\varphi'}{\varphi}f'.

Exercise 6.4 The first eigenfunction of the sphere

On the unit SnS^n, with rr the distance from the north pole, show that f=cos⁡rf = \cos r (the height function xn+1x_{n + 1}) satisfies Δf=−nf\Delta f = -nf. Check that ∣∇2f∣2=1n(Δf)2|\nabla^2f|^2 = \frac1n(\Delta f)^2, the equality case in the proof of Lichnerowicz's estimate. (On the sphere, ∇2cos⁡r=−cos⁡r g\nabla^2\cos r = -\cos r\,g.)

Solution

f′=−sin⁡rf' = -\sin r, f′′=−cos⁡rf'' = -\cos r, and Δf=−cos⁡r+(n−1)cot⁡r(−sin⁡r)=−ncos⁡r\Delta f = -\cos r + (n - 1)\cot r(-\sin r) = -n\cos r. With ∇2f=−fg\nabla^2f = -fg, ∣∇2f∣2=nf2|\nabla^2f|^2 = nf^2 and 1n(Δf)2=1nn2f2=nf2\frac1n(\Delta f)^2 = \frac1n n^2f^2 = nf^2.

Exercise 6.5 Spherical harmonics

In polar coordinates on Rn+1\mathbb{R}^{n + 1}, ΔRn+1=∂r2+nr∂r+1r2ΔSn\Delta_{\mathbb{R}^{n + 1}} = \partial_r^2 + \frac nr\partial_r + \frac{1}{r^2}\Delta_{S^n}. If PP is a harmonic polynomial, homogeneous of degree kk, write P=rkYP = r^kY with Y=P∣SnY = P|_{S^n}, and show ΔSnY=−k(k+n−1)Y\Delta_{S^n}Y = -k(k + n - 1)Y. For n=2n = 2, check that x1x2x_1x_2 is harmonic and its restriction has eigenvalue 66.

Solution

0=ΔP=(k(k−1)+nk)rk−2Y+rk−2ΔSY0 = \Delta P = (k(k - 1) + nk)r^{k - 2}Y + r^{k - 2}\Delta_SY, so ΔSY=−k(k+n−1)Y\Delta_SY = -k(k + n - 1)Y. Δ(x1x2)=0\Delta(x_1x_2) = 0 in R3\mathbb{R}^3; with k=2k = 2, n=2n = 2: 2⋅3=62\cdot3 = 6.

Exercise 6.6 The Ricci identity for 1-forms

Using the Ricci identity for vector fields and the fact that second covariant derivatives of the function ω(X)=ωkXk\omega(X) = \omega_kX^k commute, derive the identity for 1-forms.

Solution

By the product rule, ∇i∇j(ωkXk)=(∇i∇jωk)Xk+∇jωk∇iXk+∇iωk∇jXk+ωk∇i∇jXk\nabla_i\nabla_j(\omega_kX^k) = (\nabla_i\nabla_j\omega_k)X^k + \nabla_j\omega_k\nabla_iX^k + \nabla_i\omega_k\nabla_jX^k + \omega_k\nabla_i\nabla_jX^k. Antisymmetrise in i,ji, j: the left side and the two middle terms are symmetric, so 0=(∇i∇jωk−∇j∇iωk)Xk+ωkRijlkXl0 = (\nabla_i\nabla_j\omega_k - \nabla_j\nabla_i\omega_k)X^k + \omega_kR_{ijl}{}^kX^l. Renaming, (∇i∇jωk−∇j∇iωk)Xk=−RijklωlXk(\nabla_i\nabla_j\omega_k - \nabla_j\nabla_i\omega_k)X^k = -R_{ijk}{}^l\omega_lX^k for all XX.

Exercise 6.7 No spectral gap from flatness

Find λ1\lambda_1 for the flat torus R2/(aZ×bZ)\mathbb{R}^2/(a\mathbb{Z}\times b\mathbb{Z}) with a≥ba \geq b. Explain why Lichnerowicz's estimate says nothing here, and why λ1\lambda_1 can be made arbitrarily small among flat tori of area 11.

Solution

Λ∗=1aZ×1bZ\Lambda^* = \frac1a\mathbb{Z}\times\frac1b\mathbb{Z}, so λ1=4π2a2\lambda_1 = \frac{4\pi^2}{a^2}, from ξ=(1a,0)\xi = (\frac1a, 0). The estimate needs Ric⁡≥(n−1)k\operatorname{Ric} \geq (n - 1)k with k>0k > 0, and here Ric⁡=0\operatorname{Ric} = 0. With ab=1ab = 1 and a→∞a \to \infty, λ1=4π2/a2→0\lambda_1 = 4\pi^2/a^2 \to 0: a long thin torus is a slow drum.

Exercise 6.8 The Ricci tensor of a shrinking sphere

On the shrinking sphere g(t)=(1−2(n−1)t)g0g(t) = (1 - 2(n - 1)t)g_0 (9A.4 Curvature and What It Means), Ric⁡(t)=(n−1)g0\operatorname{Ric}(t) = (n - 1)g_0 does not depend on tt. Check that the right-hand side of ∂tRjk=ΔRjk+2RpjkqRpq−2RjpRpk\partial_tR_{jk} = \Delta R_{jk} + 2R_{pjkq}R^{pq} - 2R_{jp}R^p{}_k also vanishes, using the guide's Rpjkq=c−1(gpqgjk−gpkgjq)R_{pjkq} = c^{-1}(g_{pq}g_{jk} - g_{pk}g_{jq}) for g=cg0g = cg_0 of constant curvature c−1c^{-1}. What would go wrong with the opposite sign of the middle term?

Solution

Ric⁡\operatorname{Ric} is parallel, so ΔRjk=0\Delta R_{jk} = 0. With Rpq=(n−1)c−1gpqR^{pq} = (n - 1)c^{-1}g^{pq} (raising with gg): 2RpjkqRpq=2c−2(n−1)(ngjk−gjk)=2(n−1)2c−2gjk2R_{pjkq}R^{pq} = 2c^{-2}(n - 1)(ng_{jk} - g_{jk}) = 2(n - 1)^2c^{-2}g_{jk}, and 2RjpRpk=2(n−1)2c−2gjk2R_{jp}R^p{}_k = 2(n - 1)^2c^{-2}g_{jk}; they cancel. With the opposite sign the right-hand side would be −4(n−1)2c−2gjk≠0-4(n - 1)^2c^{-2}g_{jk} \neq 0, contradicting the exact solution. The sphere test fixes the sign, as in 9A.4 Curvature and What It Means.

Exercise 6.9 Rehearsal: commuting derivatives and a soliton identity

(a) Prove ∇i(∇i∇jf)=∇jΔf+Rjk∇kf\nabla^i(\nabla_i\nabla_jf) = \nabla_j\Delta f + R_{jk}\nabla^kf from the Ricci identity for 1-forms applied to ω=df\omega = df. (b) A gradient Ricci soliton is a metric with Rij+∇i∇jf=λgijR_{ij} + \nabla_i\nabla_jf = \lambda g_{ij} for a function ff and constant λ\lambda (11B.1 Ricci Solitons). Taking the trace and the divergence, and using ∇iRij=12∇jR\nabla^iR_{ij} = \frac12\nabla_jR, show Rjk∇kf=12∇jRR_{jk}\nabla^kf = \frac12\nabla_jR. (c) Deduce that R+∣∇f∣2−2λfR + |\nabla f|^2 - 2\lambda f is constant. This identity, Hamilton's, is used for every soliton in Books 11B and 12B.

Solution

(a) The Ricci identity with indices (j,i,k)(j, i, k): ∇j∇iωk−∇i∇jωk=−Rjiklωl\nabla_j\nabla_i\omega_k - \nabla_i\nabla_j\omega_k = -R_{jik}{}^l\omega_l. Contract with gikg^{ik}: ∇jΔf−∇i∇i∇jf=−gikRjikm∇mf\nabla_j\Delta f - \nabla^i\nabla_i\nabla_jf = -g^{ik}R_{jikm}\nabla^mf, using ∇jωk=∇kωj\nabla_j\omega_k = \nabla_k\omega_j to rewrite gik∇i∇jωk=∇i∇i∇jfg^{ik}\nabla_i\nabla_j\omega_k = \nabla^i\nabla_i\nabla_jf. And gikRjikm=gikRkmji=Rmjg^{ik}R_{jikm} = g^{ik}R_{kmji} = R_{mj} (contract the first and last slots). So ∇i∇i∇jf=∇jΔf+Rjm∇mf\nabla^i\nabla_i\nabla_jf = \nabla_j\Delta f + R_{jm}\nabla^mf. (b) Trace: R+Δf=nλR + \Delta f = n\lambda, so ∇jΔf=−∇jR\nabla_j\Delta f = -\nabla_jR. Divergence: 12∇jR+∇jΔf+Rjk∇kf=0\frac12\nabla_jR + \nabla_j\Delta f + R_{jk}\nabla^kf = 0, so Rjk∇kf=12∇jRR_{jk}\nabla^kf = \frac12\nabla_jR. (c) ∇j(R+∣∇f∣2−2λf)=∇jR+2∇j∇kf∇kf−2λ∇jf=∇jR+2(λgjk−Rjk)∇kf−2λ∇jf=∇jR−2Rjk∇kf=0\nabla_j(R + |\nabla f|^2 - 2\lambda f) = \nabla_jR + 2\nabla_j\nabla_kf\nabla^kf - 2\lambda\nabla_jf = \nabla_jR + 2(\lambda g_{jk} - R_{jk})\nabla^kf - 2\lambda\nabla_jf = \nabla_jR - 2R_{jk}\nabla^kf = 0.

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