19  Operators over separable Hilbert spaces

Separable Hilbert spaces are central to quantum chemistry: The space of \(N\)-electron wavefunctions, and the subspace of those wavefunctions that have finite kinetic energy are examples. Let us therefore briefly mention some types of operators that can be encountered.

19.1 Bounded operators

Definition 19.1 (Adjoint operator) Let \((V,\left\langle\cdot,\cdot\right\rangle_V)\), \((W,\left\langle\cdot,\cdot\right\rangle_W)\) be separable Hilbert spaces over \(\mathbb{F}\), and let \(T \in L(V,W)\).

The Hermitian adjoint \(T^\dag \in V(W,V)\) is the unique operator that satisfies \[\left\langle w,Tv\right\rangle_W = \left\langle T^\dag w,v\right\rangle_V\] for all \(v\in V\), \(w \in W\).

If \(H \in L(V,V)\), then \(H^\dag \in L(V,V)\) is an operator over \(V\). We say that \(H\) is Hermitian, or self-adjoint if \(H^\dag = H\).

The Hermitian adjoint generalizes the corresponding concept for finite dimensional Hilbert spaces. The Hermitian adjoint may also be defined for unbounded operators, but self-adjointness becomes a more strict concept.

19.2 Projectors

Definition 19.2 (Orthogonal projector) Let \(V\) be a separable Hilbert space over \(\mathbb{F}\). A orthogonal projector is a Hermitian (self-adjoint) \(P \in B(V)\) that satisfies \(P^2 = P\).

The set \(U = P[V]\) is a closed subspace of \(V\), and any \(v \in V\) can be uniquely decomposed as \[v = v_{\parallel} + v_{\bot},\] where \(v_\parallel = Pv \in U\) and \(\left\langle v_\parallel,v_\bot\right\rangle = 0\). We have \(v_\bot = v - v_\parallel\), and Pythagoras’ Theorem \[\|v\|^2 = \|v_\parallel\|^2 + \|v_\bot\|^2.\] A projection onto the \(x_1x_2\)-plane in \(\mathbb{R}^3\) is illustrated in Figure 19.1.

Figure 19.1: Illustration of projection in \(\mathbb{R}^3\)

19.3 Spectral theorem

Self-adjointness (equal to Hermiticity for bounded operators) allow the important Spectral Theorem, which for bounded operators goes as follows:

Theorem 19.1 (Spectral theorem for bounded self-adjoint operators) Let \(V\) be a complex separable Hilbert space, and let \(T \in L(V)\) be self-adjoint. The spectrum is real, \(\sigma(T) \subset \mathbb{R}\), and compact. We have \[\|T\|_{L(V)} = \sup\{ |\lambda| \mid \lambda \in \sigma(T) | \}.\] Moreover, \(T\) can be decomposed using what is called a spectral measure \(E\) on the real line \(\mathbb{R}\), defined on the Borel subsets of \(\mathbb{R}\), such that

\[ T = \int_{\mathbb{R}} \lambda dE(\lambda). \tag{19.1}\]

This integral represents \(T\) in terms of a integral over the spectrum of \(T\), where \(\lambda\) represents the possible spectral values (e.g., eigenvalues), and \(E(\lambda)\) acts as a projection operator that captures how much of Hilbert space corresponds to each value \(\lambda\). (For each Borel subset of \(\mathbb{R}\), such as an interval \(I\), the integral \(\int_I dE(\lambda)\) is a projection operator that projects onto the eigenspaces, ina generalized sense.)

The spectral decomposition Equation 19.1 is immensely useful. It can be used to apply functions to the operator to build new operators with well-defined properties, similarly to what one can do in finite dimensions:

Theorem 19.2 (Spectral calculus) Let \(V\) be a complex separable Hilbert spae, and let \(T \in L(V)\) be self-adjoint with spectral decomposition given by Equation 19.1. Let \(f : \mathbb{R}\to \mathbb{C}\) be any Borel measurable function. We can define a new operator \(f(T)\) by the formula \[f(T) = \int_\mathbb{R}f(\lambda) dE(\lambda).\]

Example 19.1 (Solving the time-dependent Schrödinger equation) Suppose \(V\) is the complex separable Hilbert space of quantum states of a nonrelativistic quantum system, and suppose \(H \in L(V)\) is the governing Hamiltonian operator, i.e., the time-dependent Schrödinger equation reads \[i\hbar \frac{d}{dt} \psi(t) = H\psi(t), \quad \psi(0) = \psi_0.\] This is an initial value problem and an ordinary differential equation in Hilbert space. (When \(H\) is written out it often becomes a partial differential equation formulated in Sobolev spaces.) We have not really defined what we mean by this equation in the infinite dimensional case. However, the spectral theorem allows us to write \[H = \int_{\mathbb{R}} \lambda dE(\lambda),\] and we can define a unitary operator by the formula \[U(t) = \exp(-iH t/\hbar).\] This operator is well-defined. Assuming that formal differentiation with respect to time works out as in finite dimensional spaces, we see that \[\psi(t) = U(t)\psi_0\] solves the time-dependent Schrödinger equation.

For unbounded operators over a separable Hilbert space, self-adjointness is not the same as Hermiticity. The spectral theorem and spectral calculus can be extended to unbounded operators, but is more technical.

19.4 Unitary operators

Definition 19.3 (Unitary operator) Let \(V\) be a separable Hilbert space over \(\mathbb{F}\), and let \(U \in L(V)\). We say that \(U\) is unitary if, for every \(u,v\in V\), \[\left\langle Tu,Tv\right\rangle = \left\langle u,v\right\rangle.\]

An example of a unitary operator is given in Example 19.1.

19.5 Hilbert Sobolev spaces

The Sobolev spaces \(W^{k,2}(\Omega)\):

Definition 19.4 (The spaces \(H^k(\Omega)\) and \(H^k_0(\Omega)\)) The Sobolev spaces \(W^{k,2}(\Omega)\) are denoted \(H^k(\Omega)\). Similarly, \(W^{k,2}_0(\Omega) = H^k_0(\Omega)\). They are Hilbert spaces with inner product: \[\left\langle u,v\right\rangle_{H^k} = \left\langle u,v\right\rangle_{L^2} + \sum_{\alpha, |\alpha|\leq k} \left\langle\partial_\alpha u, \partial_\alpha v\right\rangle,\] where the sum over \(\alpha\) again is a sum over partial derivatives of order \(\leq k\).

The special case \(k=1\), \[\left\langle u,v\right\rangle_{H^1} = \left\langle u,v\right\rangle_{L^2} + \left\langle\nabla u, \nabla v\right\rangle_{L^2}.\]

Remark 19.1 (Kinetic energy and Sobolev spaces). In quantum mechanics, the kinetic energy operator is \(\hat{T} = -\frac{1}{2}\nabla^2\), an unbounded but Hermitian operator. When supplied with the domain \(D(\hat{T}) = H^2_0\), then it is in fact self-adjoint.

Suppose \(u \in H^1_0(\Omega)\). Then we see that \[\left\langle u,\hat{T} u\right\rangle = \frac{1}{2} \left\langle\nabla u, \nabla u\right\rangle < +\infty.\] Here, we assumed that integration by parts is allowed with the weak derivative. Indeed it is in \(H^1_0(\Omega)\)! Thus, \(H^1_0(\Omega)\) is precisely the set of normalizable wavefuctions that has finite kinetic energy and vanish at \(\partial \Omega\). This is one of the main steps of the “weak formulation” of the Schrödinger equation.