[Nakahara GTP] 12.1 Elliptic operators and Fredholm operators
This article is one of Manifold, Differential Geometry, Fibre Bundle.
12.1.1 Elliptic operators
Let E and F be complex vector bundles over a manifold M. A differential operator D is a linear map \begin{align}D:\Gamma(M,E)\rightarrow \Gamma(M,F).\end{align} Take a chart U of M over which E and F are trivial. We denote the local coordinates of U as x^\mu. We introduce the following multi-index notation, M\equiv (\mu_1,\mu_2,\cdots,\mu_m)\quad \mu_j\in\mathbb{Z},\ \mu_j\ge 0\\ |M|\equiv \mu_1+\mu_2+\cdots+\mu_m\\ D_M=\frac{\partial^{|M|}}{\partial x^M}\equiv \frac{\partial^{\mu_1+\cdots+\mu_m}}{\partial(x^1)^{\mu_1}\cdots\partial(x^m)^{\mu_m}}. If \dim E=k and \dim F=k', the most general form of D is \begin{align}[Ds(x)]^\alpha=\sum_{|M|\le N,\ 1\le a\le k}A^{M\alpha}_a(x)D_Ms^a(x)\quad 1\le a\le k'\end{align} where s(x) is a section of E. Note that x denotes a point whose coordinates are x^\mu. This slight abuse simplifies the notation. A^M\equiv (A^M)^\alpha_a is a k\times k' matrix which may depend on the position x. The positice integer N in (2) is called the order of D. We are interseted in the case in which N=1 (the Dirac operator) and N=2 (the Laplacian). For example, if F is a spin bundle over M, the Dirac operator D\equiv i\gamma^\mu\partial_\mu+m:\ \Gamma(M,E)\rightarrow \Gamma(M,E) acts on a section \psi(x) of E as [D\psi(x)]^\alpha=i(\gamma^\mu)^\alpha_\beta\partial_\mu\psi^\beta(x)+m\psi^\alpha(x).
The symbol of D is a k\times k' matrix \begin{align}\sigma(D,\xi)\equiv \sum_{|M|=N}A^{M\alpha}_a(x)\xi_M\end{align} where \xi is a real m-tuple \xi=(\xi_1,\cdots,\xi_m). The symbol is also defined independently of the coordinates as follows. Let \pi:E\rightarrow m be a vector bundle and let p\in M, \xi\in T^*_pM and s\in \pi^{-1}_E(p). Take a section \tilde{s}\in\Gamma(M,E) such that \tilde{s}(p)=s and a function f\in \mathcal{F}(M) such that f(p)=0 and df(p)=\xi\in T^*_pM. Then the symbol may be defined by \begin{align}\sigma(D,\xi)s=\frac{1}{N!}D(f^N\tilde{s})|_p.\end{align} The factor f^N automatically picks up the Nth-order term due to the condition f(p)=0. Equation (4) yields the same symbol as (3). (Differential at a point and given order)
If the matrix \sigma(D,\xi) is invertible for each x\in M and each \xi\in \mathbb{R}^m-\{0\}, the operator D is said to be elliptic. Clearly this definition makes sense only when k=k' (square matrix). If should be noted that the symbol for a composite operator D=D_1\circ D_2 is a composite of the symbols, namely \sigma(D,\xi)=\sigma(D_1,\xi)\, \sigma(D_2,\xi). This shows that composites of elliptic operators are also elliptic. In general, powers and roots of elliptic operators are elliptic.
Example 12.1. Let x^\mu be the natural coordinates in \mathbb{R}^m. If E and F are real line bundles over \mathbb{R}^m, the Laplacian \Delta:\Gamma(\mathbb{R}^m,E)\rightarrow \Gamma(\mathbb{R}^m,F) is defined by \begin{align}\Delta\equiv \frac{\partial^2}{\partial(x^1)^2}+\cdots+\frac{\partial^2}{\partial(x^m)^2}.\end{align}
A^M is m\times 1 matrix. According to (3), the symbol is \sigma(\Delta,\xi)=\sum_\mu(\xi_\mu)^2. This is in agreement with the result obtained from (4), \sigma(\Delta,\xi)s=\frac{1}{2}\Delta(f^2\tilde{s})|_p=\frac{1}{2}\sum\frac{\partial^2}{\partial(x^\mu)^2}(f^2\tilde{s})|_p\\ =\frac{1}{2}\left. \left( f^2\Delta\tilde{s}+2f\Delta f\tilde{s}+2f\sum \frac{\partial f}{\partial x^\mu}\frac{\partial\tilde{s}}{\partial x^\mu}+2\sum\frac{\partial f}{\partial x^\mu}\frac{\partial f}{\partial x^\mu}\tilde{s}\right)\right|_p\\ =\sum(\xi_\mu)^2s. (Use f(p)=0, df=\xi) This symbol is clearly invertible for \xi\ne 0, and hence \Delta is elliptic.
12.1.2 Fredholm operators
Let D:\Gamma(M,E)\rightarrow \Gamma(M,F) be an elliptic operator. The kernel of D is the set of null eigenvectors \begin{align}\ker D\equiv \{s\in \Gamma(M,E)|Ds=0\}.\end{align} Suppose E ans F are endowed with fibre metrics, which will be denoted \langle\ ,\ \rangle_E and \langle\ ,\ \rangle_F, respectively. The adjoint D^\dagger:\Gamma(M,F)\rightarrow \Gamma(M,E) of D is defined by \begin{align}\langle s',Ds\rangle_F\equiv \langle D^\dagger s',s\rangle_E\end{align} where s\in \Gamma(M,E) and s'\in \Gamma(M,F). We defined the cokernel of D by \begin{align}\mbox{coker}D\equiv \Gamma(M,F)/\mbox{im} D.\end{align}
Among elliptic operators we are interested in a class of operators whose kernels and cokernels are finite dimensional. An elliptic operator D which satisfies this condition is called a Fredholm operator. The analytical index \begin{align}\mbox{ind}D\equiv \dim \ker D-\dim \mbox{coker}D\end{align} is well defined for a Fredholm operator. Henceforth, we will be concerned only with Fredholm operators. It is known from the general theory of operators that elliptic operators on a compact manifold are Fredholm operators. Theorem 12.1 shows that \mbox{ind}D is also expressed as \begin{align}\mbox{ind}D=\dim\ker D-\dim\ker D^\dagger.\end{align}
Theorem 12.1. Let D:\Gamma(M,E)\rightarrow \Gamma(M,F) be a Fredholm operator. Then \begin{align}\mbox{coker}D\simeq \ker D^\dagger\equiv \{s\in\Gamma(M,F)|D^\dagger s=0\}.\end{align}
Proof. Let [s]\in\mbox{coker} D be given by [s]=\{s'\in \Gamma(M,F)|s'=s+Du,\ u\in\Gamma(M,E)\}. We show that there is a surjection \ker D^\dagger\rightarrow \mbox{coker} D, namely ans [s]\in\mbox{coker}D has a representative s_0\in\ker D^\dagger. Define s_0 by \begin{align}s_0\equiv s-D\frac{1}{D^\dagger D}D^\dagger s.\end{align} We find s_0\in\ker D^\dagger since D^\dagger s_0=D^\dagger s-D^\dagger D(D^\dagger D)^{-1}D^\dagger s=D^\dagger s-D^\dagger s=0. Next, let s_0,s_0'\in\ker D^\dagger and s_0\ne s_0'. We show that [s_0]\ne [s_0'] in \Gamma(M,F)/\mbox{im}D. If [s_0]=[s_0'], there is an element u\in\Gamma(M,E) such that s_0-s_0'=Du. Then 0=\langle u,D^\dagger(s_0-s_0')\rangle_E=\langle u,D^\dagger Du\rangle_E=\langle Du,Du\rangle_F\ge 0, hence Du=0, which contradicts our assumption s_0\ne s_0'. Thus, the map s_0\mapsto [s] is a bijection and we have established that \mbox{coker}D\simeq \ker D^\dagger.
12.1.3 Elliptic complexes
Consider a sequence of Fredholm operators, \begin{align}\cdots\rightarrow \Gamma(M,E_{i-1})\stackrel{D_{i-1}}{\rightarrow}\Gamma(M,E_i)\stackrel{D_i}{\rightarrow}\Gamma(M,E_{i+1})\stackrel{D_{i+1}}{\rightarrow}\cdots\end{align} where \{E_i\} is a sequence of vector bundles over a compact manifold M. The sequence (E_i,D_i) is called an elliptic complex if D_i is nilponent (that is D_i\circ D_{i-1}=0) for any i. The reader may refer to \Gamma(M,E_i)=\Omega_i(M) and D_i=d (exterior derivative) for example. The adjoint of D_i:\Gamma(M,E_i)\rightarrow \Gamma(M,E_{i+1}) is denoted by D^\dagger_i:\Gamma(M,E_{i+1})\rightarrow\Gamma(M,E_i). The Laplacian \Delta_i:\Gamma(M,E_i)\rightarrow \Gamma(M,E_i) is \begin{align}\Delta_i\equiv D_{i-1}D^\dagger_{i-1}+D^\dagger_iD_i.\end{align} The Hodge decomposition also applies to the present case, \begin{align}s_i=D_{i-1}s_{i-1}+D^\dagger_is_{i+1}+h_i\end{align} where s_{i\pm1}\in\Gamma(M,E_{i\pm1}) and h_i is in the kernel of \Delta_i, \Delta_ih_i=0.
Analogously to the de Rham cohomology groups, we define \begin{align}H^i(E,D)\equiv \ker D_i/\mbox{im}D_{i-1}.\end{align} As in the case of de Rham theory, it can be shown that H^i(E,D) is isomorphic to the kernel of \Delta_i. Accordingly, we have \begin{align}\dim H^i(E,D)=\dim \mbox{Harm}^i(E,D)\end{align} where \mbox{Harm}^i(E,D) is a vector space spanned by \{h_i\}. The index of this elliptic complex is defined by \begin{align}\mbox{ind}D\equiv \sum^m_{i=0}(-1)^i\dim H^i(E,D)=\sum^m_{i=0}(-1)^i\dim \ker \Delta_i.\end{align} The index thus defined generalizes the Euler characteristic, see example 12.2.
How is this related to (10)? Consider the complex \Gamma(M,E)\stackrel{D}{\rightarrow}\Gamma(M,F). We may formally add zero on both sides, \begin{align}0\stackrel{i}{\hookrightarrow} \Gamma(M,E)\stackrel{D}{\rightarrow}\Gamma(M,F)\stackrel{\varphi}{\rightarrow} 0\end{align} where i is the inclusion. The index according to (19) is \dim\ker D-\{\dim\Gamma(M,F)-\dim\mbox{im}D\}=\dim\ker D-\dim\mbox{coker}D where we have noted that \dim\mbox{im}i=0, \ker\varphi=\Gamma(M,F) and \mbox{coker}D=\ker\varphi/\mbox{im}D. Thus, (19) yields the same index as (10).
It is often convenient to work with a two-term elliptic complex which has the same index as the original elliptic complex (E,D). This rolloing up is carried out by defining \begin{align}E_+\equiv \oplus_r E_{2r},\ E_-\equiv \oplus_r E_{2r+1}\end{align} which are called the even bundle and the odd bundle, respectively. Correspondingly we consider the operators \begin{align}A\equiv \oplus_r (D_{2r}+D^\dagger_{2r-1}),\ A^\dagger\equiv \oplus_r (D_{2r+1}+D^\dagger_{2r}).\end{align} We readily verify that A:\Gamma(M,E_+)\rightarrow \Gamma(M,E_-) and A^\dagger:\Gamma(M,E_-)\rightarrow \Gamma(M,E_+). From A and A^\dagger, we construct the two Laplaticans \begin{align}\Delta_+\equiv A^\dagger A=\oplus_{r,s}(D_{2r+1}+D^\dagger_{2r})(D_{2s}+D^\dagger_{2s-1})\nonumber \\ =\oplus_r(D_{2r-1}D^\dagger_{2r-1}+D^\dagger_{2r}D_{2r})=\oplus_r\Delta_{2r} \\ \Delta_-\equiv AA^\dagger = \oplus_r\Delta_{2r+1}.\end{align} Then we have \begin{align}\mbox{ind}(E_\pm,A)=\dim\ker \Delta_+-\dim\ker\Delta_-\nonumber\\ =\sum(-1)^r\dim\ker \Delta_r=\mbox{ind}(E,D).\end{align}
Example 12.2. Let us consider the de Rham complex \Omega(M) over a compact manifold M without a boundary, \begin{align}0\stackrel{i}{\rightarrow}\Omega^0(M)\stackrel{d}{\rightarrow}\Omega^1(M)\stackrel{d}{\rightarrow}\cdots \stackrel{d}{\rightarrow}\Omega^m(M)\stackrel{d}{\rightarrow}0\end{align} where m=\dim M and d stands for d_r:\Omega^r(M)\rightarrow \Omega^{r+1}(M). H^r(E,D) defined by (25) agrees with the de Rham cohomology group H_r(M,\mathbb{R}). The index is identified with the Euler characteristic, \begin{align}\mbox{ind}(\Omega^*(M),d)=\sum^m_{r=0}(-1)^r\dim H^r(M;\mathbb{R})=\chi(M).\end{align} We found in chapter 7 that b^r\equiv \dim H^r(M,\mathbb{R}) agrees with the number of linearly independent harmonic r-forms: \dim H^r(M,\mathbb{R})=\dim\mbox{Harm}^r(M)=\dim\ker\Delta_r, where \Delta_r is the Laplacian \begin{align}\Delta_r=(d+d^\dagger)^2=d_{r-1}d^\dagger_{r-1}+d^\dagger_r d_r\end{align} d^\dagger_r:\Omega^{r+1}(M)\rightarrow \Omega^r(M) being the adjoint of d_r. Now we find that \begin{align}\chi(M)=\sum^m_{r=0}(-1)^r\dim\ker\Delta_r.\end{align} This relation is very interesting since the LHS is a purely topological quantity which can be computed by triangulating M, for example, while the RHS is given by the solution of an analytic equation \Delta_ru=0. We noted in example 11.6 that \chi(M) is given by integrating the Euler class over M:\chi(M)=\int_Me(TM). Now (28) reads \begin{align}\sum^m_{r=1}(-1)^r\dim\ker \Delta_r=\int_Me(TM).\end{align} This is a typical form of the index theorem. The RHS is an analytic index while the LHS is a topological index given by the integral of certain characteristic classes. In section 12.3, we derive (29) from the Atiyah-Singer index theorem.
The two-term complex is given by \begin{align}\Omega^+(M)\equiv \oplus_r\Omega^{2r}(M)\quad \Omega^-(M)\equiv \oplus_r\Omega^{2r+1}(M).\end{align} The corresponding operators are \begin{align}A\equiv \oplus_r(d_{2r}+d^\dagger_{2r-1})\quad A^\dagger\equiv \oplus_r(d_{2r-1}+d^\dagger_{2r}).\end{align} It is left as an exercise to show that \begin{align}\mbox{ind}(\Omega^\pm(M),A)=\dim\ker A_+-\dim\ker A_-=\chi(M).\end{align}