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3: Quantum Mechanics

  • Page ID
    540241
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    • 3.1: Quantum Operators Represent Classical Variables
      This page describes the correspondence principle in quantum mechanics, stating that every classical observable has a corresponding quantum operator. It discusses observables like position and momentum, represented by operators acting on the wavefunction. Key operators include those for kinetic energy, potential energy, and the Hamiltonian, which combines both energy types. Additionally, a table outlines various quantum operators alongside their observables, emphasizing their mathematical forms.
    • 3.2: Eigenfunctions of Operators are Orthogonal
      This page explains Hermitian operators in quantum mechanics, highlighting that they correspond to experimental observables with real eigenvalues and orthogonal eigenstates. It discusses the orthogonality of eigenfunctions, proving that wavefunctions from different eigenvalues are orthogonal, illustrated with particle-in-a-box examples. The text also addresses degenerate eigenstates and their potential non-orthogonality, which can be rectified through the Gram-Schmidt Orthogonalization process.
    • 3.3: Commuting Operators Allow Infinite Precision
      This page explains the Heisenberg Uncertainty Principle and commutation relations in quantum mechanics, highlighting the significance of operators and their commutation. It details conditions for operator commutation and illustrates with examples, particularly regarding angular momentum. The text concludes that non-commuting operators impose limitations on the uncertainties of measurable physical quantities.
    • 3.4: The Quantum Mechanical Free Particle
      The simplest system in quantum mechanics has the potential energy V=0 everywhere. This is called a free particle since it has no forces acting on it. We consider the one-dimensional case, with motion only in the x-direction. We discuss that the wavefunction can be a linear combination of eigenfunctions and wavepackets can be constructed of eigenstates to generate a localized particle picture that a single eigenstate does not posess.
    • 3.5: The Energy Levels of a Rigid Rotor
      This page covers the rigid rotor in classical and quantum mechanics, emphasizing the fixed distances in the rotor approximation and the separation of variables in solving the 3D Schrödinger Equation. It discusses angular variables and derives solutions as Associated Legendre Functions, highlighting energy levels' quantization and degeneracy linked to quantum numbers. The relationship between increasing \(J\) and energy spacing is explored, challenging classical rotation concepts.
    • 3.6: The Variational Method
      In this section we introduce the powerful and versatile variational method and use it to improve the approximate solutions we found for the helium atom using the independent electron approximation.
    • 3.7: Linear Variational Method and the Secular Determinant
      A special type of variation widely used in the study of molecules is the so-called linear variation function, a linear combination of N linearly independent functions (often atomic orbitals). Quite often a trial wavefunction is expanded as a linear combination of other functions (not the eigenvalues of the Hamiltonian, since they are not known) .
    • 3.8: Perturbation Theory Expresses the Solutions in Terms of Solved Problems
      Perturbation theory is the single most important method of solving problems in quantum mechanics, and is widely used in atomic physics, condensed matter and particle physics. Perturbation theory is another approach to finding approximate solutions to a problem, by starting from the exact solution of a related, simpler problem. A critical feature of the technique is a middle step that breaks the problem into "solvable" and "perturbation" parts.
    • 3.9: Electron Spin, Indistinguishability and Slater Determinants
      This lecture address two unique aspects of electrons: spin and indistinguishability and how they couple into describing multi-electron wavefunctions.  The spin results in an angular momentum that follows the same properties of orbital angular moment including commutators and uncertainty effect.  The Slater determinant wavefunction is introduced as a way to consistently address both properties.
    • 3.10: Band Structure
      Band Theory was developed with some help from the knowledge gained during the quantum revolution in science. In 1928, Felix Bloch had the idea to take the quantum theory and apply it to solids. In 1927, Walter Heitler and Fritz London discovered bands- very closely spaced orbitals with not much difference in energy.


    This page titled 3: Quantum Mechanics is shared under a not declared license and was authored, remixed, and/or curated by Jonathan Gutow.

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