Author Archives: Pengfei

Mathematics.
Dynamics.

Notes. Some basic terms

1. Let R be a commutative ring, S be a multiplicatively closed subset in the sense that a,b\in S \Rightarrow ab \in S. Then we consider the localization S^{-1}R as the quotient S\times R/\sim, where (r,a)\sim (s,b) if (br-as)t=0 for some t\in S.

Let f\in R. We can construct a m.c.subset S=\{f^n: n\ge 0\}, and denote the corresponding local ring by R_f=S^{-1}R.

Let p\triangleleft R be a prime ideal of R. Then S=R\backslash p is m.c. We denote the corresponding local ring by R_p=S^{-1}R.

Let \text{Spec}R be the set of all prime ideals of R. For each ideal I\triangleleft R, let V_I=\{p\in \text{Spec}R: p\supset I\}. The Zariski topology on \text{Spec}R is defined that the closed subsets are exactly \{V_I: I\triangleleft R\}.

A basis for the Zariski topology on \text{Spec}R can be constructed as follows. For each f\in R, let D_f\subset \text{Spec}R to be the set of prime ideals not containing f. Then each D_f= \text{Spec}R\backslash V_{(f)} is open.

The points corresponding to maximal ideals m \triangleleft R are closed points in the sense that the singleton \{m\}=V_m.

In the case R=C[x_1, \dots, x_n], we see that each maximal ideal m=\langle x_1-a_1,\dots, x_n-a_n \rangle corresponds to a point (a_1,\dots, a_n)\in C^n. So one can interprat this as C^n \subset X= \text{Spec} R. A non-max prime ideal p (a non-closed point) corresponds an affine variety P, which is a closed subset in C^n. Then p is called the generic point of the varity P.

2. Let (M,\omega) be a symplectic manifold, G be a Lie group acting on M via symplectic diffeomorphisms. Let \mathfrak{g} be the Lie algebra of G. Each \xi \in \mathfrak{g} induces a vector field \rho(\xi):x\in M \mapsto \frac{d}{dt}\Big|_{t=0}\Big(\exp(t\xi)\cdot x\Big). Note that \rho(g^{-1}\xi g)=g_\ast \rho(\xi), and \rho([\xi,\eta])=[\rho(\xi),\rho(\eta)].

Consider the 1-form induced by the contraction \iota_{\rho(\xi)}\omega. Clearly this 1-form is closed: d\iota_{\rho(\xi)}\omega=L_{\rho(\xi)}\omega=0 since G preserves the form \omega.

Then the action is called weakly Hamiltonian, if for every \xi\in \mathfrak{g}, the one-form \iota_{\rho(\xi)} \omega is exact: \iota_{\rho(\xi)} \omega=dH_\xi for some smooth function H_{\xi} on M. Although H_\xi is only determined up to a constant C_\xi, the constant \xi \mapsto C_\xi can be chosen such that the map \xi\mapsto H_\xi becomes linear.

The action is called Hamiltonian, if the map \mathfrak{g} \to C^\infty(M), \xi\mapsto H_\xi is a Lie algebra homomorphism with respect to Poisson structure. Then \rho(\xi)=X_{H_\xi} and H_{g^{-1}\xi g}(x)=H_\xi(gx).

A moment map for a Hamiltonian G-action on (M,\omega) is a map \mu: M\to \mathfrak{g}^\ast such that H_\xi(x)=\mu(x)\cdot \xi for all \xi\in \mathfrak{g}. In other words, for each fixed point x\in M, the map \xi \mapsto H_\xi(x) from \mathfrak{g} to \mathbb{R} is a linear functional on \mathfrak{g} and is denoted by \mu(x). Also note that \mu(gx)\cdot \xi=H_\xi(gx)=H_{g^{-1}\xi g}(x). So \mu(gx)=g\mu(x)g^{-1}.

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There is no positively expansive homeomorphism

Let f be a homeomorphism on a compact metric space (X,d). Then f is said to be \mathbb{Z}-expansive, if there exists \delta>0 such that for any two points x,y\in X, if d(f^nx,f^ny)<\delta for all n\in\mathbb{Z}, then x=y. The constant \delta is called the expansive constant of f.

Similarly one can define \mathbb{N}-expansiveness if f is not invertible. An interesting phenomenon observed by Schwartzman states that

Theorem. A homeomorphism f cannot be \mathbb{N}-expansive (unless X is finite).

This result was reported in Gottschalk–Hedlund’s book Topological Dynamics (1955), and a proof was given in King’s paper A map with topological minimal self-joinings in the sense of del Junco (1990). Below we copied the proof from King’s paper.

Proof. Suppose on the contrary that there is a homeo f on (X,d) that is \mathbb{N}-expansive. Let \delta>0 be the \mathbb{N}-expansive constant of f, and d_n(x,y)=\max\{d(f^k x, f^k y): 1\le k\le n\}.

It follows from the \mathbb{N}-expansiveness that N:=\sup\{n\ge 1: d_n(x,y)\le\delta \text{ for some } d(x,y)\ge\delta\} is a finite number. Pick \epsilon\in(0,\delta) such that d_N(x,y)<\delta whenever d(x,y)<\epsilon.

Claim. If d(x,y)<\epsilon, then d(f^{-n} x, f^{-n}y)<\delta for any n\ge 1.

Proof of Claim. If not, we can prolong the N-string since f^{k}=f^{k+n}\circ f^{-n}.

Recall that a pair (x,y) is said to be \epsilon-proximal, if d(f^{n_i}x, f^{n_i}y)<\epsilon for some n_i\to\infty. The upshot for the above claim is that any \epsilon-proximal pair is \delta-indistinguishable: d(f^{n}x, f^{n}y)<\delta for all n.

Cover X by open sets of radius < \epsilon, and pick a finite subcover, say \{B_i:1\le i\le I\}. Let E=\{x_j:1\le j\le I+1\} be a subset consisting of I+1 distinct points. Then for each n\ge 0, there are two points in f^n E share the room B_{i(n)}, say f^nx_{a(n)}, and f^nx_{b(n)}. Pick a subsequence n_i such that a(n_i)\equiv a and b(n_i)\equiv b. Clearly x_a\neq x_b, and d(f^{n_i}x_a,f^{n_i}x_b)<\epsilon. Hence the pair (x_a,x_b) is \epsilon-proximal and \delta-indistinguishable. This contradicts the \mathbb{N}-expansiveness assumption on f. QED.

Area under holomorphic maps

Let f be a map from (x,y)\in \mathbb{R}^2 to (a,b)\in \mathbb{R}^2. The area form dA=dx\wedge dy gives the Jacobian dA=da\wedge db= J(x,y)dx\wedge dy, where J(x,y)=a_xb_y- a_yb_x.

Now consider the complex setting, where \displaystyle dA=\frac{i}{2} dz\wedge d\bar z. Let f be a map from z\in \mathbb{C} to w\in \mathbb{C}. Then \displaystyle dA=\frac{i}{2} dw\wedge d\bar w= \frac{i}{2}f'(z)\overline{f'(z)} dz\wedge d\bar z. So this time the Jacobian J(z) becomes f'(z)\overline{f'(z)}.

Suppose \displaystyle f(z)=\sum_{n\ge 0} a_n z^n is a holomorphic map on the unit disk D. Then
\displaystyle J(z)=\sum_{n,m\ge 0}nm a_n \bar a_m z^{n-1} \bar z^{m-1}, the area of f(D) is \displaystyle \int_D J_f(z) dA.

Using polar coordinate, we have dA= rdr\, d\theta, \displaystyle z^{n-1} \bar z^{m-1}=r^{n+m-2}e^{i\theta(n-m)},
and \displaystyle \int_D r^{n+m-2}e^{i\theta(n-m)} rdr\, d\theta= 0 if n\neq m, and =\frac{\pi}{n} if n=m.

So \displaystyle |f(D)|=\sum_{n\ge 0} n^2 |a_n|^2\cdot \frac{\pi}{n}=\pi \sum_{n\ge 0} n |a_n|^2.

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An interesting lemma about the Birkhoff sum

A few days ago I attended a lecture given by Amie Wilkinson. She presented a proof of Furstenberg’s theorem on the Lyapunov exponents of random products of matrices in SL(2,\mathbb{R}).

Let \lambda be a probability measure on SL(2,\mathbb{R}), \mu=\lambda^{\mathbb{N}} be the product measure on \Omega=SL(2,\mathbb{R})^{\mathbb{N}}. Let \sigma be the shift map on \Omega, and A:\omega\in\Omega\mapsto \omega_0\in SL(2,\mathbb{R}) be the projection. We consider the induced skew product (f,A) on \Omega\times \mathbb{R}^2. The (largest) Lyapunov exponent of (f,A) is defined to be the value \chi such that \displaystyle \lim_{n\to\infty}\frac{1}{n}\log\|A_n(\omega)\|=\chi for \mu-a.e. \omega\in \Omega.

To apply the ergodic theory, we first assume \int\log\|A\| d\lambda < \infty. Then \chi(\lambda) is well defined. There are cases when \chi(\lambda)=0:

(1) the generated group \langle\text{supp}\lambda\rangle is compact;

(2) there exists a finite set \mathcal{L}=\{L_1,\dots, L_k\} of lines that is invariant for all A\in \langle\text{supp}\lambda\rangle.

Furstenberg proved that the above cover all cases with zero exponent:
\chi(\lambda) > 0 for all other \lambda.

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Symplectic and contact manifolds

Let (M,\omega) be a symplectic manifold. It said to be exact if \omega=d\lambda for some one-form \lambda on M.

(1) If \omega=d\lambda is exact, then there is a canonical isomorphism between the v.f. and 1-forms. In particular, there exists a v.f. X such that \lambda=i_X\omega. Then we have \lambda(X)=\omega(X,X)=0, and L_X\lambda=i_X d\lambda+d i_X\lambda=i_X\omega +0=\lambda, and L_X\omega=d i_X\omega=d\lambda=\omega.

(2) Suppose there exists a vector field X on M such that its Lie-derivative L_X\omega=\omega (notice the difference with L_X\omega=0). Then Cartan’s formula says that \omega=i_X d\omega+ di_X\omega=d\lambda, where \lambda=i_X\omega. So \omega=d\lambda is exact, and L_X\lambda=i_Xd\lambda+di_X\lambda=i_X\omega+0=\lambda.

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Collections

10. Let f_a:S^1\to S^1, a\in[0,1] be a strictly increasing family of homeomorphisms on the unit circle, \rho(a) be the rotation number of f_a. Poincare observed that \rho(a)=p/q if and only if f_a admits some periodic points of period q. In this case f_a^q admits fixed points.

Note that a\mapsto \rho(a) is continuous, and non-decreasing. However, \rho may not be strictly increasing. In fact, if \rho(a_0)=p/q and f^q\neq Id, then \rho is locked at p/q for a closed interval I_{p/q}\ni a_0. More precisely, if f^q(x) > x for some x, then \rho(a)=p/q on [a_0-\epsilon,a_0] for some \epsilon > 0; if f^q(x)  0; while a_0\in \text{Int}(I_{p/q}) if both happen.

Also oberve that if r=\rho(a)\notin \mathbb{Q}, then I_r is a singelton. So assuming f_a is not unipotent for each a\in[0,1], the function a\mapsto \rho(a) is a Devil’s staircase: it is constant on closed intervals I_{p/q}, whose union \bigcup I_{p/q} is dense in I.

9. Let X:M\to TM be a vector field on M, \phi_t:M\to M be the flow induced by X on M. That is, \frac{d}{dt}\phi_t(x)=X(\phi_t(x)). Then we take a curve s\mapsto x_s\in M, and consider the solutions \phi_t(x_s). There are two ways to take derivative:

(1) \displaystyle \frac{d}{dt}\phi_t(x_s)=X(\phi_t(x_s)).

(2) \displaystyle \frac{d}{ds}\phi_t(x_s)=D\phi_t(\frac{d}{ds}x_s)), which induces the tangent flow D\phi_t:TM\to TM of \phi_t:M\to M.

Combine these two derivatives together:

\displaystyle \frac{d}{dt}D_x\phi_t(x_s')=\frac{d}{dt}\frac{d}{ds}\phi_t(x_s) =\frac{d}{ds}\frac{d}{dt}\phi_t(x_s)=\frac{d}{ds}X(\phi_t(x_s)) =D_{\phi_t(x)}X\circ D_x\phi_t(x_s').

This gives rise to an equation \displaystyle \frac{d}{dt}D_x\phi_t=D_{\phi_t(x)}X\circ D_x\phi_t.

 

Formally, one can consider the differential equation along a solution x(t):
\displaystyle \frac{d}{dt}D(t)=D_{\phi_t(x)}X\circ D(t), D(0)=Id. Then D(t) is called the linear Poincare map along x(t). Suppose x(T)=x(0). Then D(T) determines if the periodic orbit is hyperbolic or elliptic. Note that the path D(t), 0\le t\le T contains more information than the above characterization.

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The real decay rate

Let f be a C^2 uniform expanding map on the 1-torus \mathbb{T}, \mu be the unique ACIP of f, which is exponentially mixing. That is, there exists \lambda\in(0,1) such that |C(\phi,\psi,f^n)|\le C\lambda^n for any two Lipschitz functions \phi,\psi on \mathbb{T}, where
C(\phi,\psi,f^n,\mu)=\int \phi\circ f^n\cdot \psi d\mu -\mu(\phi)\cdot\mu(\psi) be the correlation function.

Let h be a C^2 diffeomorphism on \mathbb{T}, g=h^{-1}fh be the induced map, and h_\ast \nu=\mu. The new correlation function

C(\phi,\psi,g^n,\nu)=\int \phi\circ g^n\cdot \psi d\nu-\nu(\phi)\cdot\nu(\psi)
=\int \hat\phi\circ f^n(hx)\cdot \hat\psi(hx) d\nu-\nu(\phi)\cdot\nu(\psi)
=\int \hat\phi\circ f^n \cdot \hat\psi d\mu-\mu(\hat\phi)\cdot\mu(\hat\psi),

where \hat\phi=\phi\circ h^{-1}. Therefore, the two smoothly conjugate systems (g,\nu) and (f,\mu) have the same mixing rate.

Assuming h is close to identity, we see that g=h^{-1}fh is also C^2 uniformly expanding, and one may derive the mixing rate of (g,\nu) independently. However, this new rate may be different (better or worse) from \lambda. For example, f could be the linear expanding ones and archive the best possible rate among its conjugate class. Could one detect this rate from (g,\nu) itself?

In the general case, two expanding maps on \mathbb{T} are only topologically conjugate (via full shifts). So it is possible that the decay rate varies in the topologically conjugate classes.

 

Dynamics of the Weil-Petersson flow: basic geometry of the Weil-Petersson metric II

Disquisitiones Mathematicae

In the first post of this series, we planned to discuss in the third and fourth posts the proof of the following ergodicity criterion for geodesic flows in incomplete negatively curved manifolds of Burns-Masur-Wilkinson:

Theorem 1 (Burns-Masur-Wilkinson) Let $latex {N}&fg=000000$ be the quotient $latex {N=M/Gamma}&fg=000000$ of a contractible, negatively curved, possibly incomplete, Riemannian manifold $latex {M}&fg=000000$ by a subgroup $latex {Gamma}&fg=000000$ of isometries of $latex {M}&fg=000000$ acting freely and properly discontinuously. Denote by $latex {overline{N}}&fg=000000$ the metric completion of $latex {N}&fg=000000$ and $latex {partial N:=overline{N}-N}&fg=000000$ the boundary of $latex {N}&fg=000000$.Suppose that:

  • (I) the universal cover $latex {M}&fg=000000$ of $latex {N}&fg=000000$ is geodesically convex, i.e., for every $latex {p,qin M}&fg=000000$, there exists an unique geodesic segment in $latex {M}&fg=000000$ connecting $latex {p}&fg=000000$ and $latex {q}&fg=000000$.
  • (II) the metric completion $latex {overline{N}}&fg=000000$ of $latex {(N,d)}&fg=000000$ is compact.
  • (III) the boundary $latex {partial N}&fg=000000$ is volumetrically cusplike, i.e., for…

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Dynamics of the Weil-Petersson flow: basic geometry of the Weil-Petersson metric I

Disquisitiones Mathematicae

Today we will define the Weil-Petersson (WP) metric on the cotangent bundle of the moduli spaces of curves and, after that, we will see that the WP metric satisfies the first three items of the ergodicity criterion of Burns-Masur-Wilkinson (stated as Theorem 3 in the previous post).

In particular, this will “reduce” the proof of the Burns-Masur-Wilkinson theorem (of ergodicity of WP flow) to the verification of the last three items of Burns-Masur-Wilkinson ergodicity criterion for the WP metric and the proof of the Burns-Masur-Wilkinson ergodicity criterion itself.

We organize this post as follows. In next section we will quickly review some basic features of the moduli spaces of curves. Then, in the subsequent section, we will start by recalling the relationship between quadratic differentials on Riemann surfaces and the cotangent bundle of the moduli spaces of curves. After that, we will introduce the Weil-Petersson and the Teichmüller metrics…

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Dynamics of the Weil-Petersson flow: Introduction

Disquisitiones Mathematicae

Boris Hasselblatt and Françoise Dal’bo are organizing the event “Young mathematicians in Dynamical Systems” at CIRM (Luminy/Marseille, France) from November 25 to 29, 2013.

This event is part of the activities around the chaire Jean-Morlet of Boris Hasselblatt. Among the topics scheduled in this event, there is a mini-course by Keith Burns and myself around the dynamics of the Weil-Petersson (WP) geodesic flow.

In our mini-course, Keith and I plan to cover some aspects of Burns-Masur-Wilkinson theorem on the ergodicity of WP flow and, maybe, some points of our joint work with Masur and Wilkinson on the rates of mixing of WP flow.

In order to help me prepare my talks, I thought it could be a good idea to make my notes available on this blog.

So, this post starts a series of 6 posts (vaguely corresponding the 6 lectures of the mini-course) on the dynamics of…

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