Max Diem

Quantum Mechanical Foundations of Molecular Spectroscopy


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= mv, is substituted in quantum mechanics by the differential operator ModifyingAbove p With Ì‚, defined by

      The form of Eq. (2.2) can be made plausible from equations of classical wave mechanics, de Broglie's equation (Eq. [1.10]) and Planck's equation (Eq. [1.7]), but cannot be derived axiomatically. It was the genius of E. Schrödinger to realize that the substitution described in Eq. (2.2) yields differential equations that had long been known and had solutions that agreed with experiments. In the Schrödinger equations to be discussed explicitly in the next chapters (for the H atom, the vibrations and rotations of molecules, and molecular electronic energies), the classical kinetic energy T given by

      is, therefore, substituted by

      (2.4)ModifyingAbove upper T With Ì‚ equals minus StartFraction normal h with stroke squared Over 2 m EndFraction StartFraction partial-differential squared Over partial-differential x squared EndFraction

      (2.5)upper E Subscript total Baseline equals upper T plus upper V equals minus StartFraction normal h with stroke squared Over 2 m EndFraction StartFraction partial-differential squared Over partial-differential x squared EndFraction plus upper V

      (2.6)ModifyingAbove upper A With Ì‚ phi equals a phi

      where a are the eigenvalues and ϕ the corresponding eigenfunctions. The terms “operator,” “eigenvalues,” and “eigenfunctions” are terminology from linear algebra and will be further explained in Section 2.3 where the first real eigenvalue problem, the particle in a box, will be discussed. Notice that the eigenfunctions often are polynomials, and each of these eigenfunctions has its corresponding eigenvalue.

      In this book, following generally accepted notations, the total energy operator is generally identified by the symbol ModifyingAbove upper H With Ì‚ and referred to as the Hamilton operator, or the Hamiltonian, of the system. With the definition of the Hamiltonian above, it is customary to write the total energy equation of the system as

      Postulate 4: The expectation value of an observable a, associated with an operator ModifyingAbove upper A With Ì‚, for repeated measurements, is given by

      If the wavefunctions Ψ(x, t) are normalized, Eq. (2.7) simplifies to

      Postulate 5: The eigenfunctions ϕi, which are the solutions of the equation ModifyingAbove upper A With Ì‚ phi equals a phi, form a complete orthogonal set of functions or, in other words, define a vector space. This, again, will be demonstrated in Section 2.3 for the particle‐in‐a‐box wavefunctions, which are all orthogonal to each other and therefore may be considered unit vectors in a vector