Sum rule in quantum mechanics

In quantum mechanics, a sum rule is a formula for transitions between energy levels, in which the sum of the transition strengths is expressed in a simple form. Sum rules are used to describe the properties of many physical systems, including solids, atoms, atomic nuclei, and nuclear constituents such as protons and neutrons.

The sum rules are derived from general principles, and are useful in situations where the behavior of individual energy levels is too complex to be described by a precise quantum-mechanical theory. In general, sum rules are derived by using Heisenberg's quantum-mechanical algebra to construct operator equalities, which are then applied to the particles or energy levels of a system.

Derivation of sum rules[1] edit

Assume that the Hamiltonian   has a complete set of eigenfunctions   with eigenvalues  :

 

For the Hermitian operator   we define the repeated commutator   iteratively by:

 

The operator   is Hermitian since   is defined to be Hermitian. The operator   is anti-Hermitian:

 

By induction one finds:

 

and also

 

For a Hermitian operator we have

 

Using this relation we derive:

 

The result can be written as

 

For   this gives:

 

See also edit

References edit

  1. ^ Wang, Sanwu (1999-07-01). "Generalization of the Thomas-Reiche-Kuhn and the Bethe sum rules". Physical Review A. 60 (1). American Physical Society (APS): 262–266. Bibcode:1999PhRvA..60..262W. doi:10.1103/physreva.60.262. ISSN 1050-2947.