Lesson 269: Functions of Operators

Introduction: Beyond Simple Operations

What does it mean to compute \(\sin(\hat{A})\) or \(e^{\hat{A}}\) for a matrix \(\hat{A}\)? Using diagonalization and power series, we can extend ordinary functions to operators—essential for time evolution in quantum mechanics.

Definition via Power Series

For a function with Taylor expansion \(f(x) = \sum_{n=0}^{\infty} c_n x^n\):

\[f(\hat{A}) = \sum_{n=0}^{\infty} c_n \hat{A}^n\]

Examples:

Using Spectral Decomposition

If \(\hat{A} = \sum_n a_n |a_n\rangle\langle a_n|\), then:

\[f(\hat{A}) = \sum_n f(a_n) |a_n\rangle\langle a_n|\]

The function is applied to each eigenvalue!

Worked Examples

Example 1: Exponential of σ_z

\(\sigma_z = |+\rangle\langle +| - |-\rangle\langle -|\) with eigenvalues ±1:

\[e^{i\theta\sigma_z} = e^{i\theta}|+\rangle\langle +| + e^{-i\theta}|-\rangle\langle -| = \begin{pmatrix} e^{i\theta} & 0 \\ 0 & e^{-i\theta} \end{pmatrix}\]

Example 2: Exponential of Pauli Matrix

For any Pauli matrix \(\vec{\sigma} \cdot \hat{n}\) with \(|\hat{n}| = 1\):

\[e^{i\theta \vec{\sigma} \cdot \hat{n}} = \cos(\theta)I + i\sin(\theta)(\vec{\sigma} \cdot \hat{n})\]

This is a rotation by angle \(2\theta\) about axis \(\hat{n}\) on the Bloch sphere.

Example 3: Time Evolution Operator

The time evolution operator is:

\[U(t) = e^{-i\hat{H}t/\hbar}\]

If \(\hat{H}|n\rangle = E_n|n\rangle\), then:

\[U(t) = \sum_n e^{-iE_nt/\hbar}|n\rangle\langle n|\]

The Quantum Connection

Time evolution in quantum mechanics is governed by the exponential of the Hamiltonian:

\[|\psi(t)\rangle = e^{-i\hat{H}t/\hbar}|\psi(0)\rangle\]

This is why diagonalizing \(\hat{H}\) solves the time-dependence: in the energy basis, each component just rotates in phase at its own frequency \(\omega_n = E_n/\hbar\).