Skip to Content
Math401Math 401, Fall 2025: Thesis notesMath 401, Fall 2025: Thesis notes, R2, Levy's concentration theorem and Levy's family

Math 401, Fall 2025: Thesis notes, R2, Levy’s concentration theorem and Levy’s family

Progress: 2/5=40% (denominator and enumerator may change)

Levy’s concentration theorem

Tip

This version of Levy’s concentration theorem can be found in Geometry of Quantum states  15.84 and 15.85.

Our goal is to prove the generalized version of Levy’s concentration theorem used in Hayden’s work for η\eta-Lipschitz functions.

Let f:Sn−1→Rf:S^{n-1}\to \mathbb{R} be a η\eta-Lipschitz function. Let MfM_f denote the median of ff and ⟨f⟩\langle f\rangle denote the mean of ff. (Note this can be generalized to many other manifolds.)

Select a random point x∈Sn−1x\in S^{n-1} with n>2n>2 according to the uniform measure (Haar measure). Then the probability of observing a value of ff much different from the reference value is exponentially small.

Pr⁡[∣f(x)−Mf∣>ϵ]≤exp⁡(−nϵ22η2)\operatorname{Pr}[|f(x)-M_f|>\epsilon]\leq \exp(-\frac{n\epsilon^2}{2\eta^2}) Pr⁡[∣f(x)−⟨f⟩∣>ϵ]≤2exp⁡(−(n−1)ϵ22η2)\operatorname{Pr}[|f(x)-\langle f\rangle|>\epsilon]\leq 2\exp(-\frac{(n-1)\epsilon^2}{2\eta^2})

Levy’s concentration theorem via sub-Gaussian concentration

Tip

This version of Levy’s concentration theorem can be found in High-dimensional probability  5.1.4.

Isoperimetric inequality on Rn\mathbb{R}^n

Among all subsets A⊂RnA\subset \mathbb{R}^n with a given volume, the Euclidean ball has the minimal area.

That is, for any ϵ>0\epsilon>0, Euclidean balls minimize the volume of the ϵ\epsilon-neighborhood of AA.

Where the volume of the ϵ\epsilon-neighborhood of AA is defined as

Aϵ(A)≔{x∈Rn:∃y∈A,∥x−y∥2≤ϵ}=A+ϵB2nA_\epsilon(A)\coloneqq \{x\in \mathbb{R}^n: \exists y\in A, \|x-y\|_2\leq \epsilon\}=A+\epsilon B_2^n

Here the ∥⋅∥2\|\cdot\|_2 is the Euclidean norm. (The theorem holds for both geodesic metric on sphere and Euclidean metric on Rn\mathbb{R}^n.)

Isoperimetric inequality on the sphere

Let σn(A)\sigma_n(A) denotes the normalized area of AA on nn dimensional sphere SnS^n. That is σn(A)≔Area⁡(A)Area⁡(Sn)\sigma_n(A)\coloneqq\frac{\operatorname{Area}(A)}{\operatorname{Area}(S^n)}.

Let ϵ>0\epsilon>0. Then for any subset A⊂SnA\subset S^n, given the area σn(A)\sigma_n(A), the spherical caps minimize the volume of the ϵ\epsilon-neighborhood of AA.

The above two inequalities is not proved in the Book High-dimensional probability. But you can find it in the Appendix C of Gromov’s book Metric Structures for Riemannian and Non-Riemannian Spaces.

To continue prove the theorem, we use sub-Gaussian concentration (Chapter 3 of High-dimensional probability by Roman Vershynin) of sphere nSn\sqrt{n}S^n.

This will leads to some constant C>0C>0 such that the following lemma holds:

The “Blow-up” lemma

Let AA be a subset of sphere nSn\sqrt{n}S^n, and σ\sigma denotes the normalized area of AA. Then if σ≥12\sigma\geq \frac{1}{2}, then for every t≥0t\geq 0,

σ(At)≥1−2exp⁡(−ct2)\sigma(A_t)\geq 1-2\exp(-ct^2)

where At={x∈Sn:dist⁡(x,A)≤t}A_t=\{x\in S^n: \operatorname{dist}(x,A)\leq t\} and cc is some positive constant.

Proof of the Levy’s concentration theorem

Proof:

Without loss of generality, we can assume that η=1\eta=1. Let MM denotes the median of f(X)f(X).

So Pr⁡[∣f(X)≤M∣]≥12\operatorname{Pr}[|f(X)\leq M|]\geq \frac{1}{2}, and Pr⁡[∣f(X)≥M∣]≥12\operatorname{Pr}[|f(X)\geq M|]\geq \frac{1}{2}.

Consider the sub-level set A≔{x∈nSn:∣f(x)∣≤M}A\coloneqq \{x\in \sqrt{n}S^n: |f(x)|\leq M\}.

Since Pr⁡[X∈A]≥12\operatorname{Pr}[X\in A]\geq \frac{1}{2}, by the blow-up lemma, we have

Pr⁡[X∈At]≥1−2exp⁡(−ct2)\operatorname{Pr}[X\in A_t]\geq 1-2\exp(-ct^2)

And since

Pr⁡[X∈At]≤Pr⁡[f(X)≤M+t]\operatorname{Pr}[X\in A_t]\leq \operatorname{Pr}[f(X)\leq M+t]

Combining the above two inequalities, we have

Pr⁡[f(X)≤M+t]≥1−2exp⁡(−ct2)\operatorname{Pr}[f(X)\leq M+t]\geq 1-2\exp(-ct^2)

Levy’s concentration theorem via Levy family

Levy’s concentration theorem (Gromov’s version)

The Levy’s lemma can also be found in Metric Structures for Riemannian and Non-Riemannian Spaces by M. Gromov. 312.193\frac{1}{2}.19 The Levy concentration theory.

Theorem 312.193\frac{1}{2}.19 Levy concentration theorem:

An arbitrary 1-Lipschitz function f:Sn→Rf:S^n\to \mathbb{R} concentrates near a single value a0∈Ra_0\in \mathbb{R} as strongly as the distance function does.

That is

μ{x∈Sn:∣f(x)−a0∣≥ϵ}<κn(ϵ)≤2exp⁡(−(n−1)ϵ22)\mu\{x\in S^n: |f(x)-a_0|\geq\epsilon\} < \kappa_n(\epsilon)\leq 2\exp(-\frac{(n-1)\epsilon^2}{2})

where

κn(ϵ)=∫ϵπ2cos⁡n−1(t)dt∫0π2cos⁡n−1(t)dt\kappa_n(\epsilon)=\frac{\int_\epsilon^{\frac{\pi}{2}}\cos^{n-1}(t)dt}{\int_0^{\frac{\pi}{2}}\cos^{n-1}(t)dt}

a0a_0 is the Levy mean of function ff, that is the level set of f−1:R→Snf^{-1}:\mathbb{R}\to S^n divides the sphere into equal halves, characterized by the following equality:

μ(f−1(−∞,a0])≥12 and μ(f−1[a0,∞))≥12\mu(f^{-1}(-\infty,a_0])\geq \frac{1}{2} \text{ and } \mu(f^{-1}[a_0,\infty))\geq \frac{1}{2}

Hardcore computing may generates the bound but M. Gromov did not make the detailed explanation here.

Detailed proof by Takashi Shioya.

The central idea is to draw the connection between the given three topological spaces, S2n+1S^{2n+1}, CPnCP^n and R\mathbb{R}.

First, we need to introduce the following distribution and lemmas/theorems:

OBSERVATION

consider the orthogonal projection from Rn+1\mathbb{R}^{n+1}, the space where SnS^n is embedded, to Rk\mathbb{R}^k, we denote the restriction of the projection as πn,k:Sn(n)→Rk\pi_{n,k}:S^n(\sqrt{n})\to \mathbb{R}^k. Note that πn,k\pi_{n,k} is a 1-Lipschitz function (projection will never increase the distance between two points).

We denote the normalized Riemannian volume measure on Sn(n)S^n(\sqrt{n}) as σn(⋅)\sigma^n(\cdot), and σn(Sn(n))=1\sigma^n(S^n(\sqrt{n}))=1.

Definition of Gaussian measure on Rk\mathbb{R}^k

We denote the Gaussian measure on Rk\mathbb{R}^k as γk\gamma^k.

dγk(x)≔12πkexp⁡(−12∥x∥2)dxd\gamma^k(x)\coloneqq\frac{1}{\sqrt{2\pi}^k}\exp(-\frac{1}{2}\|x\|^2)dx

x∈Rkx\in \mathbb{R}^k, ∥x∥2=∑i=1kxi2\|x\|^2=\sum_{i=1}^k x_i^2 is the Euclidean norm, and dxdx is the Lebesgue measure on Rk\mathbb{R}^k.

Basically, you can consider the Gaussian measure as the normalized Lebesgue measure on Rk\mathbb{R}^k with standard deviation 11.

Maxwell-Boltzmann distribution law

It is such a wonderful fact for me, that the projection of n+1n+1 dimensional sphere with radius n\sqrt{n} to Rk\mathbb{R}^k is a Gaussian distribution as n→∞n\to \infty.

For any natural number kk,

d(πn,k)∗σn(x)dx→dγk(x)dx\frac{d(\pi_{n,k})_*\sigma^n(x)}{dx}\to \frac{d\gamma^k(x)}{dx}

where (πn,k)∗σn(\pi_{n,k})_*\sigma^n is the push-forward measure of σn\sigma^n by πn,k\pi_{n,k}.

In other words,

(πn,k)∗σn→γk weakly as n→∞(\pi_{n,k})_*\sigma^n\to \gamma^k\text{ weakly as }n\to \infty

Proof

We denote the nn dimensional volume measure on Rk\mathbb{R}^k as vol⁡k\operatorname{vol}_k.

Observe that πn,k−1(x),x∈Rk\pi_{n,k}^{-1}(x),x\in \mathbb{R}^k is isometric to Sn−k(n−∥x∥2)S^{n-k}(\sqrt{n-\|x\|^2}), that is, for any x∈Rkx\in \mathbb{R}^k, πn,k−1(x)\pi_{n,k}^{-1}(x) is a sphere with radius n−∥x∥2\sqrt{n-\|x\|^2} (by the definition of πn,k\pi_{n,k}).

So,

d(πn,k)∗σn(x)dx=vol⁡n−k(πn,k−1(x))vol⁡k(Sn(n))=(n−∥x∥2)n−k2∫∥x∥≤n(n−∥x∥2)n−k2dx\begin{aligned} \frac{d(\pi_{n,k})_*\sigma^n(x)}{dx}&=\frac{\operatorname{vol}_{n-k}(\pi_{n,k}^{-1}(x))}{\operatorname{vol}_k(S^n(\sqrt{n}))}\\ &=\frac{(n-\|x\|^2)^{\frac{n-k}{2}}}{\int_{\|x\|\leq \sqrt{n}}(n-\|x\|^2)^{\frac{n-k}{2}}dx}\\ \end{aligned}

as n→∞n\to \infty.

note that lim⁡n→∞(1−an)n=e−a\lim_{n\to \infty}{(1-\frac{a}{n})^n}=e^{-a} for any a>0a>0.

(n−∥x∥2)n−k2=(n(1−∥x∥2n))n−k2→nn−k2exp⁡(−∥x∥22)(n-\|x\|^2)^{\frac{n-k}{2}}=\left(n(1-\frac{\|x\|^2}{n})\right)^{\frac{n-k}{2}}\to n^{\frac{n-k}{2}}\exp(-\frac{\|x\|^2}{2})

So

(n−∥x∥2)n−k2∫∥x∥≤n(n−∥x∥2)n−k2dx=e−∥x∥22∫x∈Rke−∥x∥22dx=1(2π)k2e−∥x∥22=dγk(x)dx\begin{aligned} \frac{(n-\|x\|^2)^{\frac{n-k}{2}}}{\int_{\|x\|\leq \sqrt{n}}(n-\|x\|^2)^{\frac{n-k}{2}}dx}&=\frac{e^{-\frac{\|x\|^2}{2}}}{\int_{x\in \mathbb{R}^k}e^{-\frac{\|x\|^2}{2}}dx}\\ &=\frac{1}{(2\pi)^{\frac{k}{2}}}e^{-\frac{\|x\|^2}{2}}\\ &=\frac{d\gamma^k(x)}{dx} \end{aligned}

Proof of the Levy’s concentration theorem via the Maxwell-Boltzmann distribution law

We use the Maxwell-Boltzmann distribution law and Levy’s isoperimetric inequality to prove the Levy’s concentration theorem.

The goal is the same as the Gromov’s version, first we bound the probability of the sub-level set of ff by the κn(ϵ)\kappa_n(\epsilon) function by Levy’s isoperimetric inequality. Then we claim that the κn(ϵ)\kappa_n(\epsilon) function is bounded by the Gaussian distribution.

Note, this section is not rigorous enough in sense of mathematics and the author should add sections about Levy family and observable diameter to make the proof more rigorous and understandable.

Proof

Let f:Sn→Rf:S^n\to \mathbb{R} be a 1-Lipschitz function.

Consider the two sets of points on the sphere SnS^n with radius n\sqrt{n}:

Ω+={x∈Sn:f(x)≤a0−ϵ},Ω−={x∈Sn:f(x)≥a0+ϵ}\Omega_+=\{x\in S^n: f(x)\leq a_0-\epsilon\}, \Omega_-=\{x\in S^n: f(x)\geq a_0+\epsilon\}

Note that Ω+∪Ω−\Omega_+\cup \Omega_- is the whole sphere Sn(n)S^n(\sqrt{n}).

By the Levy’s isoperimetric inequality, we have

vol⁡n−k(πn,k−1(ϵ))≤vol⁡n−k(πn,k−1(Ω+))+vol⁡n−k(πn,k−1(Ω−))\operatorname{vol}_{n-k}(\pi_{n,k}^{-1}(\epsilon))\leq \operatorname{vol}_{n-k}(\pi_{n,k}^{-1}(\Omega_+))+\operatorname{vol}_{n-k}(\pi_{n,k}^{-1}(\Omega_-))

We define κn(ϵ)\kappa_n(\epsilon) as the following:

κn(ϵ)=vol⁡n−k(πn,k−1(ϵ))vol⁡k(Sn(n))=∫ϵπ2cos⁡n−1(t)dt∫0π2cos⁡n−1(t)dt\kappa_n(\epsilon)=\frac{\operatorname{vol}_{n-k}(\pi_{n,k}^{-1}(\epsilon))}{\operatorname{vol}_k(S^n(\sqrt{n}))}=\frac{\int_\epsilon^{\frac{\pi}{2}}\cos^{n-1}(t)dt}{\int_0^{\frac{\pi}{2}}\cos^{n-1}(t)dt}

By the Levy’s isoperimetric inequality, and the Maxwell-Boltzmann distribution law, we have

μ{x∈Sn:∣f(x)−a0∣≥ϵ}<κn(ϵ)≤2exp⁡(−(n−1)ϵ22)\mu\{x\in S^n: |f(x)-a_0|\geq\epsilon\} < \kappa_n(\epsilon)\leq 2\exp(-\frac{(n-1)\epsilon^2}{2})

Levy’s Isoperimetric inequality

This section is from the Appendix C+C_+ of Gromov’s book Metric Structures for Riemannian and Non-Riemannian Spaces.

Not very edible for undergraduates.

Differential Geometry

This section is designed for stupids like me skipping too much essential materials in the book.

This part might be extended to a separate note, let’s check how far we can go from this part.

References:

Manifold

Unexpectedly, a good definition of the manifold is defined in the topology I.

Check section 36. This topic extends to a wonderful chapter 8 in the book where you can hardly understand chapter 2.

Definition of m-manifold

An mm-manifold is a Hausdorff space XX with a countable basis (second countable) such that each point of xx of XX has a neighborhood homeomorphic to an open subset of Rm\mathbb{R}^m.

Example of second countable space

Let X=RX=\mathbb{R} and B={(a,b)∣a,b∈R,a<b}\mathcal{B}=\{(a,b)|a,b\in \mathbb{R},a<b\} (collection of all open intervals with rational endpoints).

Since the rational numbers are countable, so B\mathcal{B} is countable.

So R\mathbb{R} is second countable.

Likewise, Rn\mathbb{R}^n is also second countable.

Example of manifold

1-manifold is a curve and 2-manifold is a surface.

Theorem of imbedded space

If XX is a compact mm-manifold, then XX can be imbedded in Rn\mathbb{R}^n for some nn.

This theorem might save you from imagining abstract structures back to real dimension. Good news, at least you stay in some real numbers.

Smooth manifolds and Lie groups

This section is waiting for the completion of book Introduction to Smooth Manifolds by John M. Lee.

Partial derivatives

Let U⊆RnU\subseteq \mathbb{R}^n and f:U→Rnf:U\to \mathbb{R}^n be a map.

For any a=(a1,⋯ ,an)∈Ua=(a_1,\cdots,a_n)\in U, j∈{1,⋯ ,n}j\in \{1,\cdots,n\}, the jj-th partial derivative of FF at aa is defined as

∂f∂xj(a)=lim⁡h→0f(a1,⋯ ,aj+h,⋯ ,an)−f(a1,⋯ ,aj,⋯ ,an)h=lim⁡h→0f(a+hej)−f(a)h\begin{aligned} \frac{\partial f}{\partial x_j}(a)&=\lim_{h\to 0}\frac{f(a_1,\cdots,a_j+h,\cdots,a_n)-f(a_1,\cdots,a_j,\cdots,a_n)}{h} \\ &=\lim_{h\to 0}\frac{f(a+he_j)-f(a)}{h} \end{aligned}

Continuously differentiable maps

Let U⊆RnU\subseteq \mathbb{R}^n and f:U→Rnf:U\to \mathbb{R}^n be a map.

If for any j∈{1,⋯ ,n}j\in \{1,\cdots,n\}, the jj-th partial derivative of ff is continuous at aa, then ff is continuously differentiable at aa.

If ∀a∈U\forall a\in U, ∂f∂xj\frac{\partial f}{\partial x_j} exists and is continuous at aa, then ff is continuously differentiable on UU. or C1C^1 map. (Note that C0C^0 map is just a continuous map.)

Smooth maps

A function f:U→Rnf:U\to \mathbb{R}^n is smooth if it is of class CkC^k for every k≥0k\geq 0 on UU. Such function is called a diffeomorphism if it is also a bijection and its inverse is also smooth.

Charts

Let MM be a smooth manifold. A chart is a pair (U,φ)(U,\varphi) where U⊆MU\subseteq M is an open subset and φ:U→U^⊆Rn\varphi:U\to \hat{U}\subseteq \mathbb{R}^n is a homeomorphism (a continuous bijection map and its inverse is also continuous).

If p∈Up\in U and φ(p)=0\varphi(p)=0, then we say that pp is the origin of the chart (U,φ)(U,\varphi).

For p∈Up\in U, we note that the continuous function φ(p)=(x1(p),⋯ ,xn(p))\varphi(p)=(x_1(p),\cdots,x_n(p)) gives a vector in Rn\mathbb{R}^n. The (x1(p),⋯ ,xn(p))(x_1(p),\cdots,x_n(p)) is called the local coordinates of pp in the chart (U,φ)(U,\varphi).

Atlas

Let MM be a smooth manifold. An atlas is a collection of charts A={(Uα,ϕα)}α∈I\mathcal{A}=\{(U_\alpha,\phi_\alpha)\}_{\alpha\in I} such that M=⋃α∈IUαM=\bigcup_{\alpha\in I} U_\alpha.

An atlas is said to be smooth if the transition maps ϕα∘ϕβ−1:ϕβ(Uα∩Uβ)→ϕα(Uα∩Uβ)\phi_\alpha\circ \phi_\beta^{-1}:\phi_\beta(U_\alpha\cap U_\beta)\to \phi_\alpha(U_\alpha\cap U_\beta) are smooth for all α,β∈I\alpha, \beta\in I.

Smooth manifold

A smooth manifold is a pair (M,A)(M,\mathcal{A}) where MM is a topological manifold and A\mathcal{A} is a smooth atlas.

Fundamental group

A fundamental group of a point pp in a topological space XX is the group of all paths (continuous map f:I→Xf:I\to X, I=[0,1]⊆RI=[0,1]\subseteq \mathbb{R}) from pp to pp.

  • Product defined as composition of paths.
  • Identity element is the constant path from pp to pp.
  • Inverse is the reverse path.

smooth local coordinate representations

If MM is a smooth manifold, then any chart (U,φ)(U,\varphi) contained in the given maximal smooth atlas is called a smooth chart, and the map φ\varphi is called a smooth coordinate map because it gives a coordinate

Lie group

Lie group is a group (satisfying group axioms: closure, associativity, identity, inverses) that is also a smooth manifold. with the operator m:G×G→Gm:G\times G\to G, and the inverse operation i:G→Gi:G\to G that are both smooth.

In short, a Lie group is a group that is also a smooth manifold with map G×G→GG\times G\to G given by (g,h)↦gh−1(g,h)\mapsto gh^-1 that is smooth.

Example of Lie group

The general linear group GL(n,R)GL(n,\mathbb{R}) is the group of all n×nn\times n invertible matrices over R\mathbb{R}.

This is a Lie group since

  1. Multiplication is a smooth map GL(n,R)×GL(n,R)→GL(n,R)GL(n,\mathbb{R})\times GL(n,\mathbb{R})\to GL(n,\mathbb{R}) since it is a polynomial map.
  2. Inverse is a smooth map GL(n,R)→GL(n,R)GL(n,\mathbb{R})\to GL(n,\mathbb{R}) by cramer’s rule.

If GG is a Lie group, then any open subgroup (with subgroup topology and open set in GG) HH of GG is also a Lie group.

Translation map on Lie group

If GG is a Lie group, then the translation map Lg:G→GL_g:G\to G given by Lg(h)=ghL_g(h)=gh and Rg:G→GR_g:G\to G given by Rg(h)=hgR_g(h)=hg are both smooth and are diffeomorphisms on GG.

Derivation and tangent vectors

The directional derivative of a geometric tangent vector va∈Ranv_a\in \mathbb{R}^n_a yields a map Dv∣a:C∞(Rn)→RD_v\vert_a:C^\infty(\mathbb{R}^n)\to \mathbb{R} given by the formula

Dv∣a(f)=Dvf(a)=ddt∣t=0f(a+tva)D_v\vert_a(f)=D_v f(a)=\frac{d}{dt}\bigg\vert_{t=0}f(a+tv_a)

Note that this is a linear over R\mathbb{R}, and satisfies the product rule.

Dv∣a(f⋅g)=f(a)Dv∣a(g)+g(a)Dv∣a(f)D_v\vert_a(f\cdot g)=f(a)D_v\vert_a(g)+g(a)D_v\vert_a(f)

We can generalize this representation to the following definition:

If aa is a point of Rn\mathbb{R}^n, then a derivation at aa is a linear map w:C∞(Rn)→Rw:C^\infty(\mathbb{R}^n)\to \mathbb{R} such that it is linear over R\mathbb{R} and satisfies the product rule.

w(f⋅g)=w(f)⋅g(a)+f(a)⋅w(g)w(f\cdot g)=w(f)\cdot g(a)+f(a)\cdot w(g)

Let TaRnT_a\mathbb{R}^n denote the set of all derivations of C∞(Rn)C^\infty(\mathbb{R}^n) at aa. So TaRnT_a\mathbb{R}^n is a vector space over R\mathbb{R}.

(w1+w2)(f)=w1(f)+w2(f),(cw)(f)=c(w(f))(w_1+w_2)(f)=w_1(f)+w_2(f),\quad (cw)(f)=c(w(f))

Some key properties are given below and check the proof in the book for details.

  1. If ff is a constant function, then w(f)=0w(f)=0.
  2. If f(a)=g(a)=0f(a)=g(a)=0, then w(f⋅g)=0w(f\cdot g)=0.
  3. For each geometric tangent vector va∈Ranv_a\in \mathbb{R}^n_a, the map Dv∣a:C∞(Rn)→RD_v\vert_a:C^\infty(\mathbb{R}^n)\to \mathbb{R} is a derivation at aa.
  4. The map va↦Dv∣av_a\mapsto D_v\vert_a is an isomorphism of vector spaces from Ran\mathbb{R}^n_a to TaRnT_a\mathbb{R}^n.

Tangent vector on Manifolds

Let MM be a smooth manifold. Let p∈Mp\in M. A tangent vector to MM at pp is a derivation at pp if it satisfies:

v(f⋅g)=f(p)vg+g(p)vf∏ for all f,g∈C∞(M)v(f\cdot g)=f(p)vg+g(p)vf\prod \text{ for all } f,g\in C^\infty(M)

The set of all derivations of C∞(M)C^\infty(M) at pp is denoted by TpMT_pM is called tangent space to MM at pp. An element of TpMT_pM is called a tangent vector to MM at pp.

Tangent bundle

We define the tangent bundle of MM as the disjoint union of all the tangent spaces:

TM=⨆p∈MTpMTM=\bigsqcup_{p\in M} T_pM

We write the element in TMTM as pair (p,v)(p,v) where p∈Mp\in M and v∈TpMv\in T_pM.

The tangent bundle comes with a natural projection map π:TM→M\pi:TM\to M given by π(p,v)=p\pi(p,v)=p.

Section of map

If π:M→N\pi:M\to N is any continuous map, a section of π\pi is a continuous right inverse of π\pi. For example σ:N→M\sigma:N\to M is a section of π\pi if σ∘π=IdN\sigma\circ \pi=Id_N.

Vector field

A vector field on MM is a section of the map π:TM→M\pi:TM\to M.

More concretely, a vector field is a continuous map X:M→TMX:M\to TM, usually written p↦Xpp\mapsto X_p, with property that

π∘X=IdM\pi\circ X=Id_M

That is a map from element on the manifold to the tangent space of the manifold.

Riemannian manifolds and geometry

Riemannian metric

A Riemannian metric is a smooth assignment of an inner product to each tangent space TpMT_pM of the manifold.

More formally, let MM be a smooth manifold. A Riemannian metric on MM is a smooth covariant 2-tensor field g∈T2(M)g\in \mathcal{T}^2(M) whose value gpg_p at each p∈Mp\in M is an inner product on TpMT_p M.

Thus gg is a symmetric 2-tensor field that is positive definite in the sense that gp(v,v)≥0g_p(v,v)\geq 0 for each p∈Mp\in M and each v∈TpMv\in T_p M, with equality if and only if v=0v=0.

Riemannian metric exists in great abundance.

A good news for smooth manifold is that every smooth manifold admits a Riemannian metric.

Example of Riemannian metrics

An example of Riemannian metric is the Euclidean metric, the bilinear form of d(p,q)=∥p−q∥2d(p,q)=\|p-q\|_2 on Rn\mathbb{R}^n.

More formally, the Riemannian metric g‾\overline{g} on Rn\mathbb{R}^n at each x∈Rnx\in \mathbb{R}^n , for v,w∈TxRnv,w\in T_x \mathbb{R}^n with stardard coordinates (x1,…,xn)(x^1,\ldots,x^n) as v=∑i=1nvi∂xiv=\sum_{i=1}^n v_i \partial_x^i and $w=\sum_{

Riemannian manifolds

A Riemannian manifold is a smooth manifold equipped with a Riemannian metric, which is a smooth assignment of an inner product to each tangent space TpMT_pM of the manifold.

More formally, a Riemannian manifold is a pair (M,g)(M,g), where MM is a smooth manifold and gg is a specific choice of Riemannian metric on MM.

An example of Riemannian manifold is the sphere CPn\mathbb{C}P^n.

Notion of Connection

A connection is a way to define the directional derivative of a vector field along a curve on a Riemannian manifold.

For every p∈Mp\in M, where MM denote the manifold, suppose M=RnM=\mathbb{R}^n, then let X=(f1,⋯ ,fn)X=(f_1,\cdots,f_n) be a vector field on MM. The directional derivative of XX along the point pp is defined as

DVX=lim⁡h→0X(p+h)−X(p)hD_VX=\lim_{h\to 0}\frac{X(p+h)-X(p)}{h}

Notion of Curvatures

Note

Geometrically, the curvature of the manifold is radius of the tangent sphere of the manifold.

Nabla notation and Levi-Civita connection

Fundamental theorem of Riemannian geometry

Let (M,g)(M,g) be a Riemannian or pseudo-Riemannian manifold (with or without boundary). There exist sa unique connection ∇\nabla on TMTM that is compatible with gg and symmetric. It is called the Levi-Civita connection of gg (or also, when gg is a positive definite, the Riemannian connection).

Ricci curvature

Last updated on