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Density of states

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The density of states function, , is defined as the number of electronic states per unit energy for electron energies between and . It is represented as where is number of states occupied at energy . The energy is the highest occupied energy level, a.k.a. Fermi Energy.

The derivation[1] of for the particle in 3D box model at 0 K can be used as an approximation for electrons in the metal. The energy of a state at is given by , where is Planck’s constant, is the mass of electron, and is the box length. The number of states with is given by twice the volume of a positive octant of the sphere with radius :

,

where volume of the box. Using the definition of density of states:

The function can also be defined as, , or density of states per unit volume. Thus, the at 0K is proportional to . At finite temperatures, is modulated by Fermi-Dirac distribution.

The density of states function is important for calculations of effects based on band theory. In Fermi's Golden Rule, a calculation for the rate of optical absorption, it provides both the number of excitable electrons and the number of final states for an electron. It appears in calculations of electrical conductivity where it provides the number of mobile states, and in computing electron scattering rates where it provides the number of final states after scattering.[2]

For energies inside a band gap, g(E) = 0.

References

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  1. ^ Kittel, Charles (2005). Introduction to Solid State Physics. Hoboken, NJ: Wiley. ISBN 9780471415268.
  2. ^ Sakurai, J. J. (2010). Modern Quantum Mechanics. Pearson. ISBN 9780805382914.