Fiveable

⚛️Intro to Quantum Mechanics I Unit 4 Review

QR code for Intro to Quantum Mechanics I practice questions

4.4 Expectation values and the Ehrenfest theorem

⚛️Intro to Quantum Mechanics I
Unit 4 Review

4.4 Expectation values and the Ehrenfest theorem

Written by the Fiveable Content Team • Last updated September 2025
Written by the Fiveable Content Team • Last updated September 2025
⚛️Intro to Quantum Mechanics I
Unit & Topic Study Guides

Quantum mechanics gets real with expectation values and observables. These concepts help us predict what we'll measure in experiments, connecting the weird quantum world to our everyday experiences.

The Ehrenfest theorem bridges the gap between quantum and classical physics. It shows how quantum particles behave like classical objects on average, helping us understand the fuzzy line between these two realms.

Expectation Values and Observables

Understanding Expectation Values

  • Expectation value represents the average outcome of measuring an observable in a quantum system
  • Calculated using the formula A=ψAψdx\langle A \rangle = \int_{-\infty}^{\infty} \psi^ A \psi dx
  • Provides statistical information about quantum systems
  • Depends on the wave function and the operator associated with the observable
  • Crucial for predicting experimental results in quantum mechanics
  • Can be time-dependent for systems not in stationary states

Observables and Operators in Quantum Mechanics

  • Observable refers to a physical quantity that can be measured in a quantum system
  • Examples include position, momentum, energy, and angular momentum
  • Each observable corresponds to a Hermitian operator in quantum mechanics
  • Operators act on wave functions to produce new wave functions
  • Hermitian operators ensure real-valued expectation values
  • Eigenvalues of operators represent possible measurement outcomes
  • Measurement process collapses the wave function into an eigenstate of the measured observable

Mathematical Properties of Operators

  • Linear operators obey the superposition principle
  • Commutator of two operators defined as [A,B]=ABBA[A, B] = AB - BA
  • Non-commuting operators lead to uncertainty relations (Heisenberg uncertainty principle)
  • Commonly used operators include position operator x^=x\hat{x} = x and momentum operator p^=iddx\hat{p} = -i\hbar \frac{d}{dx}
  • Energy operator (Hamiltonian) plays a central role in the Schrödinger equation

Ehrenfest Theorem and Time Evolution

Ehrenfest Theorem Fundamentals

  • Ehrenfest theorem connects quantum expectation values to classical equations of motion
  • Describes the time evolution of expectation values for position and momentum
  • Stated mathematically as: ddtx=pm\frac{d}{dt}\langle x \rangle = \frac{\langle p \rangle}{m} ddtp=dVdx\frac{d}{dt}\langle p \rangle = -\langle \frac{dV}{dx} \rangle
  • Demonstrates that expectation values follow classical trajectories on average
  • Applies to systems with slowly varying potentials and wave packets with small spread

Time Evolution of Expectation Values

  • Time-dependent Schrödinger equation governs the evolution of quantum states
  • Expectation values change over time for non-stationary states
  • Rate of change of an expectation value given by: ddtA=1i[A,H]+At\frac{d}{dt}\langle A \rangle = \frac{1}{i\hbar}\langle [A, H] \rangle + \langle \frac{\partial A}{\partial t} \rangle
  • Commutator term represents quantum effects
  • Partial derivative term accounts for explicit time dependence of the operator
  • Time evolution preserves normalization of the wave function

Classical Limit and Correspondence Principle

Understanding the Classical Limit

  • Classical limit occurs when quantum effects become negligible
  • Typically observed for large quantum numbers or macroscopic systems
  • Wave packets become highly localized in position and momentum space
  • Uncertainty principle becomes less significant relative to measured quantities
  • Quantum interference effects diminish
  • Schrödinger equation approaches the classical Hamilton-Jacobi equation
  • Examples include high-energy particles and large-scale objects (planets, baseballs)

Correspondence Principle and its Implications

  • Correspondence principle states that quantum mechanics must reproduce classical physics in appropriate limits
  • Formulated by Niels Bohr as a guiding principle in developing quantum theory
  • Ensures consistency between quantum and classical descriptions
  • Manifests in various ways:
    • Energy levels become continuous in the limit of large quantum numbers
    • Angular momentum quantization approaches classical values for large l
    • Wave packets follow classical trajectories for macroscopic objects
  • Helps in understanding the transition between quantum and classical regimes
  • Provides a framework for interpreting quantum results in familiar classical terms