Density of states
The density of states of a physical system is defined such that is the number of states which could be occupied with an energy in the interval . In fact, need not be an energy; it should just be something that effectively identifies the state.
In its simplest form, the density of states is as follows, where is the number of states with energy less than or equal to the argument :
If the states can be treated as waves, which is often the case, then we can calculate the density of states in -space, i.e. as a function of the wavenumber . Once we have , we use the dispersion relation to find , by demanding that:
Inverting the dispersion relation to get might be difficult, in which case the left-hand equation can be satisfied numerically.
Define as the number of states with a -value less than or equal to the argument, or in other words, the volume of a hypersphere with radius . Then the -dimensional density of states has the following general form:
Where is each state’s degeneracy (e.g. due to spin), and is the smallest allowed -value, according to the characteristic length of the system. We divide by to limit ourselves to the sector where all axes are positive, because we are only considering the magnitude of .
In one dimension , the number of states within a distance from the origin is the distance from to (we let it run negative, since its meaning does not matter here), given by:
To get , we choose to look at a rod of length , across which the function is a standing wave, meaning that the allowed values of must be as follows, where :
Take the smallest option , such that , the 1D density of states is:
In 2D, the number of states within a range of the origin is the area of a circle with radius :
Analogously to the 1D case, we take the system to be a square of side , so again. The density of states then becomes:
In 3D, the number of states is the volume of a sphere with radius :
For a cube with side , we once again find . We thus get:
All these expressions contain the characteristic length/area/volume , and therefore give the number of states in that region only. Keep in mind that is free to choose; it need not be the physical size of the system. In fact, we typically want the density of states per unit length/area/volume, so we can just set in our preferred unit of distance.
If the system is infinitely large, or if it has periodic boundaries, then becomes a continuous variable and . But again, is arbitrary, so a finite value can be chosen.
- H. Gould, J. Tobochnik, Statistical and thermal physics, 2nd edition, Princeton.
- B. Van Zeghbroeck, Principles of semiconductor devices, 2011, University of Colorado.