Book 8A

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Course 8Book 8A: Smooth ManifoldsChapter 7

Tensors and Index Notation

Stress, diffusion and the notation every Ricci flow paper uses.

23 min read · Updated Oct 3, 2026

Read with Lee, Introduction to Smooth Manifolds (2nd edition), chapter 12 (tensors: multilinear algebra, symmetric and alternating tensors, tensor fields, pullbacks). Lee's Introduction to Riemannian Manifolds, chapter 2, covers raising and lowering indices with a metric; this chapter's table is the guide's own.

In this chapter · 7 sections
  1. 7.1The stress tensor
  2. 7.2Tensors
  3. 7.3The metric raises and lowers
  4. 7.4The guide's conventions
  5. 7.5Ten index computations
  6. 7.6History
  7. 7.7Exercises

Every paper on the Ricci flow is written in index notation: ∂tgij=−2Rij\partial_tg_{ij} = -2R_{ij}, ΔR=gij∇i∇jR\Delta R = g^{ij}\nabla_i\nabla_jR, ∣Rm⁡∣2=RijklRijkl|\operatorname{Rm}|^2 = R_{ijkl}R^{ijkl}. The notation is compact and powerful, and it is almost never explained in the papers, which assume it. This chapter explains it once, completely. A tensor is a multilinear function of tangent vectors and covectors (8A.3 Tangent Vectors and Bundles); in coordinates it is an array of components with upper and lower indices, transforming in a definite way when the coordinates change. The summation convention sums over each index that appears once up and once down. A metric lets you raise and lower indices, and contraction of an upper with a lower index produces quantities that don't depend on the coordinates at all.

The chapter ends with the guide's notation table and a drill of ten index computations, each of which reappears in the evolution equations of 11A.2 How Curvature Evolves. The last one, the first line of 11A.2 How Curvature Evolves, is the rehearsal.

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

  • define tensors of type (k,l)(k, l), tensor fields, symmetric and alternating tensors, and contractions;
  • read and write expressions in index notation with the summation convention;
  • use a metric to raise and lower indices, take traces and compute norms of tensors;
  • state the transformation law of a tensor's components;
  • use the guide's conventions for curvature, and check them on the round sphere.

The stress tensor

In the world Model Forces on a surface inside a material

Inside a loaded bridge girder, a pressurised tank or the Earth's crust, every small surface element feels a force from the material on its other side. Cauchy showed in the 1820s that this force depends linearly on the surface's orientation: there is a stress tensor σ\sigma such that the force per unit area (the traction) on a surface with unit normal nn is

ti=σijnj.t_i = \sigma_{ij}n^j.

In Cartesian coordinates σ\sigma is a 3×33\times3 array, and σij\sigma_{ij} is the ii-th component of the force on a face whose normal points along the jj-th axis (Figure 7.1). Balance of angular momentum makes it symmetric, σij=σji\sigma_{ij} = \sigma_{ji}, so it has three real eigenvalues, the principal stresses, along three perpendicular principal directions, where the traction is purely normal: no shear.

Engineers judge whether a ductile metal will yield by a scalar built from the stress tensor alone, the von Mises stress, which is unchanged by rotating the coordinates: σvM=32sijsij\sigma_{\mathrm{vM}} = \sqrt{\frac32s_{ij}s_{ij}}, where sij=σij−13σkkδijs_{ij} = \sigma_{ij} - \frac13\sigma_{kk}\delta_{ij} is the trace-free part (Exercise 7.3). Building such invariants by contracting indices is exactly what this chapter teaches; the scalar curvature R=gijRijR = g^{ij}R_{ij} and the norm ∣Ric⁡∣2|\operatorname{Ric}|^2 are built the same way.

Figure 7.1. Stress components on the faces of a small cube (schematic): on the face with outward normal eje_j, the traction has components σ1j,σ2j,σ3j\sigma_{1j}, \sigma_{2j}, \sigma_{3j}, one normal to the face and two shears along it.

Tensors

Let VV be a real vector space of dimension nn with dual V∗V^*. A tensor of type (k,l)(k, l) on VV is a multilinear map

T:V∗×⋯×V∗⏟k×V×⋯×V⏟l→R.T : \underbrace{V^*\times\dots\times V^*}_{k}\times\underbrace{V\times\dots\times V}_{l} \to \mathbb{R}.

A (0,1)(0, 1)-tensor is a covector, a (1,0)(1, 0)-tensor a vector (via V≅V∗∗V \cong V^{**}), a (0,2)(0, 2)-tensor a bilinear form, and a (1,1)(1, 1)-tensor a linear map V→VV \to V. Given a basis eie_i of VV and the dual basis eie^i of V∗V^* (ei(ej)=δjie^i(e_j) = \delta^i_j), TT is determined by its components

Ti1…ikj1…jl=T(ei1,…,eik,ej1,…,ejl),T^{i_1\dots i_k}{}_{j_1\dots j_l} = T(e^{i_1}, \dots, e^{i_k}, e_{j_1}, \dots, e_{j_l}),

upper indices for the covector slots, lower indices for the vector slots: nk+ln^{k+l} numbers.

On a manifold, tensors at each point TpMT_pM form the tensor bundles, and a tensor field is a smooth section: in coordinates, components Ti…j…(x)T^{i\dots}{}_{j\dots}(x) that are smooth functions, with respect to the bases ∂i\partial_i of TpMT_pM and dxidx^i of Tp∗MT_p^*M. A Riemannian metric gg is a symmetric positive definite (0,2)(0, 2)-tensor field with components gijg_{ij}; the Ricci tensor RijR_{ij} is a symmetric (0,2)(0, 2)-tensor field; the curvature tensor RijklR_{ijkl} is a (0,4)(0, 4)-tensor field (9A.4 Curvature and What It Means).

The summation convention. In a product, an index that appears once as a superscript and once as a subscript is summed from 11 to nn: viωi=∑iviωiv^i\omega_i = \sum_iv^i\omega_i, AijvjA^i{}_jv^j is the vector AvAv. An index appearing once is free, and an equation must have the same free indices, in the same positions, on both sides. An index appearing twice in the same position, as in viviv_iv_i, is a warning sign: without a metric it is meaningless.

The transformation law. Under a change of coordinates, each upper index transforms with ∂x~∂x\frac{\partial\tilde x}{\partial x} and each lower index with ∂x∂x~\frac{\partial x}{\partial\tilde x} (8A.3 Tangent Vectors and Bundles):

T~ab=∂x~a∂xi∂xj∂x~bTij,\tilde T^{a}{}_{b} = \frac{\partial\tilde x^a}{\partial x^i}\frac{\partial x^j}{\partial\tilde x^b}T^i{}_j,

and similarly for more indices. This is how one recognises that an array of functions defined in each chart is a tensor field.

Symmetric and alternating tensors. A covariant tensor is symmetric if it is unchanged by swapping any two arguments (gij=gjig_{ij} = g_{ji}), and alternating if it changes sign (ωij=−ωji\omega_{ij} = -\omega_{ji}). Alternating tensors are the differential forms of 8A.8 Differential Forms and Stokes’ Theorem. The curvature tensor has a mixture of symmetries, Rijkl=−Rjikl=−Rijlk=RklijR_{ijkl} = -R_{jikl} = -R_{ijlk} = R_{klij} (9A.4 Curvature and What It Means).

Contraction. Summing an upper index against a lower one reduces the type from (k,l)(k, l) to (k−1,l−1)(k - 1, l - 1) and gives a tensor again, independent of coordinates: the trace AiiA^i{}_i of a (1,1)(1, 1)-tensor is the trace of the linear map. Contraction is how invariants are built.

The metric raises and lowers

A metric gijg_{ij} is an invertible matrix at each point; its inverse is written gijg^{ij}:

gijgjk=δki.g^{ij}g_{jk} = \delta^i_k.

It is a symmetric (2,0)(2, 0)-tensor. Together they identify vectors and covectors:

vi=gijvj(lowering),ωi=gijωj(raising),v_i = g_{ij}v^j \quad\text{(lowering)}, \qquad \omega^i = g^{ij}\omega_j \quad\text{(raising)},

so one writes the same letter with the index in either position. The gradient of a function is dfdf with its index raised, ∇if=gij∂jf\nabla^if = g^{ij}\partial_jf (8A.3 Tangent Vectors and Bundles). Raising both indices of the Ricci tensor gives Rij=gikgjlRklR^{ij} = g^{ik}g^{jl}R_{kl}.

With raising and lowering, any two indices can be contracted. The trace of a (0,2)(0, 2)-tensor is tr⁡gh=gijhij\operatorname{tr}_gh = g^{ij}h_{ij}; for example the scalar curvature is R=gijRijR = g^{ij}R_{ij}, and tr⁡gg=gijgij=δii=n\operatorname{tr}_gg = g^{ij}g_{ij} = \delta^i_i = n. The inner product of two tensors of the same type contracts all indices pairwise,

⟨T,S⟩=gipgjqTijSpq=TijSij,∣T∣2=TijTij,\langle T, S\rangle = g^{ip}g^{jq}T_{ij}S_{pq} = T_{ij}S^{ij}, \qquad |T|^2 = T_{ij}T^{ij},

and in an orthonormal frame (gij=δijg_{ij} = \delta_{ij}) it is the sum of squares of the components. So ∣g∣2=n|g|^2 = n, and ∣Ric⁡∣2=RijRij|\operatorname{Ric}|^2 = R_{ij}R^{ij} is the sum of the squares of the eigenvalues of the Ricci tensor.

The guide's conventions

Different books use different conventions for curvature, differing by signs and the order of indices, and quoting a formula from one book into another is a classic source of errors. This guide uses one set throughout, following John Lee's Introduction to Riemannian Manifolds; Book 9A defines everything in it. Whatever the source, check a formula on the round unit sphere, where the answers are fixed:

quantity definition in this guide on the round unit SnS^n
metric, inverse gij=g(∂i,∂j)g_{ij} = g(\partial_i, \partial_j), gijgjk=δkig^{ij}g_{jk} = \delta^i_k
curvature endomorphism R(X,Y)Z=∇X∇YZ−∇Y∇XZ−∇[X,Y]ZR(X, Y)Z = \nabla_X\nabla_YZ - \nabla_Y\nabla_XZ - \nabla_{[X, Y]}Z
curvature tensor Rm⁡(X,Y,Z,W)=g(R(X,Y)Z,W)\operatorname{Rm}(X, Y, Z, W) = g(R(X, Y)Z, W), Rijkl=Rm⁡(∂i,∂j,∂k,∂l)R_{ijkl} = \operatorname{Rm}(\partial_i, \partial_j, \partial_k, \partial_l) Rijkl=gilgjk−gikgjlR_{ijkl} = g_{il}g_{jk} - g_{ik}g_{jl}
sectional curvature K(X,Y)=Rm⁡(X,Y,Y,X)∣X∣2∣Y∣2−g(X,Y)2K(X, Y) = \frac{\operatorname{Rm}(X, Y, Y, X)}{\lvert X\rvert^2\lvert Y\rvert^2 - g(X, Y)^2} K≡1K \equiv 1
Ricci tensor Rij=Rkijk=gklRkijlR_{ij} = R_{kij}{}^k = g^{kl}R_{kijl} Rij=(n−1)gijR_{ij} = (n - 1)g_{ij}
scalar curvature R=gijRijR = g^{ij}R_{ij} R=n(n−1)R = n(n - 1)
Hessian, Laplacian ∇i∇jf\nabla_i\nabla_jf, Δf=gij∇i∇jf\Delta f = g^{ij}\nabla_i\nabla_jf Δ≤0\Delta \leq 0 (the "analyst's" sign)
Ricci flow ∂tgij=−2Rij\partial_tg_{ij} = -2R_{ij} g(t)=(1−2(n−1)t)g0g(t) = (1 - 2(n - 1)t)g_0

The Laplacian here is ∑∂i2\sum\partial_i^2 in Euclidean space, with non-positive spectrum (4A.7 Compact Operators and Spectra), so the heat equation is ∂tu=Δu\partial_tu = \Delta u. Some geometry books use the opposite sign; Ricci flow papers almost always use this one.

Ten index computations

Each of the following takes a line or two and is used later; work through them with the summation convention, and check the free indices on both sides.

  1. δii=n\delta^i_i = n, and gijgij=ng^{ij}g_{ij} = n.
  2. Raising then lowering returns the original: gij(gjkωk)=δikωk=ωig_{ij}(g^{jk}\omega_k) = \delta_i^k\omega_k = \omega_i.
  3. Contraction is coordinate-independent: under the transformation law the Jacobians in TiiT^i{}_i cancel.
  4. The trace-free part of a symmetric hijh_{ij} is h˚ij=hij−tr⁡hngij\mathring h_{ij} = h_{ij} - \frac{\operatorname{tr}h}{n}g_{ij}, with tr⁡h˚=0\operatorname{tr}\mathring h = 0 and ∣h˚∣2=∣h∣2−(tr⁡h)2n|\mathring h|^2 = |h|^2 - \frac{(\operatorname{tr}h)^2}{n}.
  5. Hence ∣h∣2≥(tr⁡h)2n|h|^2 \geq \frac{(\operatorname{tr}h)^2}{n}, with equality iff hh is a multiple of gg. For the Ricci tensor: ∣Ric⁡∣2≥R2n|\operatorname{Ric}|^2 \geq \frac{R^2}{n}, the inequality behind the scalar curvature estimate of 6A.4 Maximum Principles.
  6. The inner product is symmetric and positive: ∣T∣2≥0|T|^2 \geq 0, with equality iff T=0T = 0 (compute in an orthonormal frame).
  7. The derivative of the inverse metric. Differentiating gijgjk=δkig^{ij}g_{jk} = \delta^i_k: ∂tgij gjk+gij∂tgjk=0\partial_tg^{ij}\,g_{jk} + g^{ij}\partial_tg_{jk} = 0, so ∂tgij=−gipgjq∂tgpq\partial_tg^{ij} = -g^{ip}g^{jq}\partial_tg_{pq}.
  8. The derivative of the determinant. ∂tlog⁡det⁡(gij)=gij∂tgij\partial_t\log\det(g_{ij}) = g^{ij}\partial_tg_{ij} (Jacobi's formula, Exercise 7.4). So the volume element dV=det⁡g dxdV = \sqrt{\det g}\,dx changes by ∂tdV=12gij∂tgij dV\partial_tdV = \frac12g^{ij}\partial_tg_{ij}\,dV.
  9. Under Ricci flow ∂tgij=−2Rij\partial_tg_{ij} = -2R_{ij}, item 8 gives ∂tdV=−R dV\partial_tdV = -R\,dV: volume shrinks where the scalar curvature is positive, and the total volume of a closed manifold evolves by ddtVol⁡=−∫R dV\frac{d}{dt}\operatorname{Vol} = -\int R\,dV.
  10. Contracting a symmetric with an antisymmetric tensor gives zero: if Sij=SjiS_{ij} = S_{ji} and Aij=−AjiA^{ij} = -A^{ji}, then SijAij=0S_{ij}A^{ij} = 0 (relabel i↔ji \leftrightarrow j).
In the world Data Diffusion tensor imaging of the brain

Water diffuses through brain tissue, and in white matter it moves faster along nerve fibres than across them, because fibre membranes and myelin hinder sideways motion. Peter Basser, James Mattiello and Denis Le Bihan showed in 1994 that MRI can measure the full diffusion tensor DijD_{ij} at each point: a symmetric positive definite 3×33\times3 tensor, the coefficient in the anisotropic diffusion equation ∂tc=∂i(Dij∂jc)\partial_tc = \partial_i(D^{ij}\partial_jc) (6A.5 Weak Solutions and Elliptic Regularity). Its eigenvectors give the directions of fastest and slowest diffusion, and its eigenvalues the rates; it is pictured as an ellipsoid at each point, elongated along the fibres (Figure 7.2). Following the principal eigenvector from point to point traces the fibre pathways, tractography, first demonstrated by Susumu Mori and colleagues in the rat brain in 1999. The scalar used most in clinical studies, the fractional anisotropy, is built from the eigenvalues by contractions of the kind in item 4: it is zero for an isotropic tensor and approaches 11 for diffusion along a single direction.

Figure 7.2. Diffusion tensors drawn as ellipses along a curved fibre bundle (a synthetic example, computed): inside the bundle the principal eigenvector follows the fibres and the tensor is strongly anisotropic; outside it is nearly isotropic. Tractography follows the long axes (orange curve).
In the world Model The tennis-racket theorem

A rigid body's resistance to rotation is the inertia tensor IijI_{ij}, a symmetric positive definite tensor whose eigenvectors are the principal axes. Spinning a body about the axis of largest or smallest moment of inertia is stable; about the intermediate axis it is unstable, and the body flips periodically. Toss a tennis racket or a phone spinning about the axis across its face, in the plane of the face, and it comes back turned over. The phenomenon follows from Euler's equations for rigid-body rotation, written in the principal frame, where the inertia tensor is diagonal; it is especially striking in weightlessness, where a spinning wing nut has been filmed flipping again and again aboard space stations.

Where this goes The first line of the evolution equations

11A.2 How Curvature Evolves computes how every geometric quantity evolves under the Ricci flow. It begins with the inverse metric (item 7 with ∂tgpq=−2Rpq\partial_tg_{pq} = -2R_{pq}), the volume form (item 9), then the Christoffel symbols, the curvature tensor, the Ricci tensor and the scalar curvature. Every step is an index computation of the kind in this chapter, with covariant derivatives (9A.2 Connections) in place of partial derivatives. Fluency here is the difference between following those computations and being lost in them.

History

Cauchy introduced the stress tensor in 1822–27. The calculus of components transforming by Jacobians, the absolute differential calculus, was developed by Gregorio Ricci-Curbastro from 1884 and set out with Tullio Levi-Civita in 1900; Einstein, who learned it from Marcel Grossmann, introduced the summation convention in 1916 in his foundation of general relativity, and the subject became known as tensor calculus. The coordinate-free view of tensors as multilinear maps became standard in the twentieth century. Diffusion tensor imaging dates from 1994 and tractography from 1999.

Recall Where we stand

A tensor of type (k,l)(k, l) is a multilinear map on kk covectors and ll vectors, with components carrying kk upper and ll lower indices that transform by Jacobians; tensor fields are smooth families of them. Repeated upper–lower indices are summed; contraction gives coordinate-free quantities. A metric gijg_{ij} with inverse gijg^{ij} raises and lowers indices, defines traces gijhijg^{ij}h_{ij} and norms ∣T∣2=TijTij|T|^2 = T_{ij}T^{ij}. The guide's curvature conventions follow Lee and are checked on the unit sphere: Ric⁡=(n−1)g\operatorname{Ric} = (n - 1)g, R=n(n−1)R = n(n - 1). Under Ricci flow, ∂tgij=2Rij\partial_tg^{ij} = 2R^{ij} and ∂tdV=−R dV\partial_tdV = -R\,dV. 8A.8 Differential Forms and Stokes’ Theorem studies the alternating tensors: differential forms and Stokes' theorem.

Exercises

Exercise 7.1 The inverse metric

Show that gijgjk=δkig^{ij}g_{jk} = \delta^i_k determines gijg^{ij}, that it is symmetric, and that it transforms as a (2,0)(2, 0)-tensor. For the polar-coordinate metric dr2+r2dθ2dr^2 + r^2d\theta^2, write gijg_{ij} and gijg^{ij}.

Solution

(gij)(g^{ij}) is the inverse matrix of (gij)(g_{ij}), unique and symmetric because gg is. If g~ab=JiaJjbgij\tilde g_{ab} = J^i{}_aJ^j{}_bg_{ij} with J=∂x/∂x~J = \partial x/\partial\tilde x, then the inverse is g~ab=(J−1)ai(J−1)bjgij\tilde g^{ab} = (J^{-1})^a{}_i(J^{-1})^b{}_jg^{ij}, the (2,0)(2, 0) law. Polar: g=diag⁡(1,r2)g = \operatorname{diag}(1, r^2), g−1=diag⁡(1,r−2)g^{-1} = \operatorname{diag}(1, r^{-2}).

Exercise 7.2 Norms in an orthonormal frame

For a symmetric 2-tensor hh with eigenvalues λ1,…,λn\lambda_1, \dots, \lambda_n with respect to gg (the eigenvalues of hijh^i{}_j), show tr⁡h=∑λi\operatorname{tr}h = \sum\lambda_i and ∣h∣2=∑λi2|h|^2 = \sum\lambda_i^2. Deduce item 5 from the Cauchy–Schwarz inequality.

Exercise 7.3 The von Mises stress

For the uniaxial stress σ=diag⁡(σ0,0,0)\sigma = \operatorname{diag}(\sigma_0, 0, 0), compute the trace-free part ss, sijsijs_{ij}s_{ij}, and show σvM=∣σ0∣\sigma_{\mathrm{vM}} = |\sigma_0|. For pure shear, σ12=σ21=τ\sigma_{12} = \sigma_{21} = \tau and all other components zero, show σvM=3∣τ∣\sigma_{\mathrm{vM}} = \sqrt3|\tau|.

Solution

Uniaxial: trace σ0\sigma_0, s=diag⁡(23,−13,−13)σ0s = \operatorname{diag}(\frac23, -\frac13, -\frac13)\sigma_0, sijsij=69σ02=23σ02s_{ij}s_{ij} = \frac69\sigma_0^2 = \frac23\sigma_0^2, so σvM=32⋅23∣σ0∣=∣σ0∣\sigma_{\mathrm{vM}} = \sqrt{\frac32\cdot\frac23}|\sigma_0| = |\sigma_0|. Shear: trace 00, s=σs = \sigma, sijsij=2τ2s_{ij}s_{ij} = 2\tau^2, σvM=3∣τ∣\sigma_{\mathrm{vM}} = \sqrt3|\tau|.

Exercise 7.4 Jacobi's formula

Show that ddtdet⁡A(t)=det⁡A⋅tr⁡(A−1A˙)\frac{d}{dt}\det A(t) = \det A\cdot\operatorname{tr}(A^{-1}\dot A) for invertible A(t)A(t). (At A=IA = I, det⁡(I+tB)=1+ttr⁡B+O(t2)\det(I + tB) = 1 + t\operatorname{tr}B + O(t^2); reduce the general case to it.) Deduce item 8.

Exercise 7.5 The sphere check

Using the table's formula Rijkl=gilgjk−gikgjlR_{ijkl} = g_{il}g_{jk} - g_{ik}g_{jl} for the unit sphere, compute Rij=gklRkijlR_{ij} = g^{kl}R_{kijl} and R=gijRijR = g^{ij}R_{ij}, and the sectional curvature of a pair of orthonormal vectors. (You should get (n−1)gij(n - 1)g_{ij}, n(n−1)n(n - 1) and 11.)

Solution

gklRkijl=gkl(gklgij−gkjgil)=ngij−δjlgil=ngij−gijg^{kl}R_{kijl} = g^{kl}(g_{kl}g_{ij} - g_{kj}g_{il}) = ng_{ij} - \delta^l_jg_{il} = ng_{ij} - g_{ij}. Then R=gij(n−1)gij=n(n−1)R = g^{ij}(n - 1)g_{ij} = n(n - 1). For orthonormal X=e1X = e_1, Y=e2Y = e_2: Rm⁡(e1,e2,e2,e1)=g11g22−g12g21=1\operatorname{Rm}(e_1, e_2, e_2, e_1) = g_{11}g_{22} - g_{12}g_{21} = 1.

Exercise 7.6 Rehearsal: the evolution of the inverse metric and the volume

Under the Ricci flow ∂tgij=−2Rij\partial_tg_{ij} = -2R_{ij}: (a) show ∂tgij=2Rij\partial_tg^{ij} = 2R^{ij}, using item 7; (b) show ∂tdV=−R dV\partial_tdV = -R\,dV, using item 8; (c) for the round sphere g(t)=(1−2(n−1)t)g0g(t) = (1 - 2(n - 1)t)g_0, check both directly (RijR^{ij} at time tt is computed with g(t)g(t)). This is the first line of 11A.2 How Curvature Evolves.

Solution

(a) ∂tgij=−gipgjq(−2Rpq)=2Rij\partial_tg^{ij} = -g^{ip}g^{jq}(-2R_{pq}) = 2R^{ij}. (b) ∂tdV=12gij(−2Rij)dV=−R dV\partial_tdV = \frac12g^{ij}(-2R_{ij})dV = -R\,dV. (c) With λ=1−2(n−1)t\lambda = 1 - 2(n - 1)t: gij=λ−1g0ijg^{ij} = \lambda^{-1}g_0^{ij}, so ∂tgij=2(n−1)λ−2g0ij\partial_tg^{ij} = 2(n - 1)\lambda^{-2}g_0^{ij}; and Rpq=(n−1)g0,pqR_{pq} = (n - 1)g_{0,pq} (scale-invariant), so Rij=gipgjqRpq=(n−1)λ−2g0ijR^{ij} = g^{ip}g^{jq}R_{pq} = (n - 1)\lambda^{-2}g_0^{ij}. Volume: dV=λn/2dV0dV = \lambda^{n/2}dV_0, ∂tdV=n2λn/2−1(−2(n−1))dV0=−n(n−1)λdV\partial_tdV = \frac n2\lambda^{n/2-1}(-2(n - 1))dV_0 = -\frac{n(n - 1)}{\lambda}dV, and R=n(n−1)λR = \frac{n(n - 1)}{\lambda}.

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