Next: Justification of real-space O(N)
Up: A comparison of linear
Previous: Introduction
Tight binding
There are already many descriptions of tight binding available in the
literature[12,13,14,15,16,17], which will not be
repeated here. For now we note the following which will be referred to
frequently in the forthcoming sections. The cohesive energy
(Ucoh) is given by:
|
Ucoh = Uband+Urep-Uatoms
|
(1) |
where Uband is the band energy, the calculation of which is the focus of
this paper, Urep is a repulsive energy, generally given as a sum of
pair potentials, and Uatoms is the total one electron energy of the
free atoms.
The band energy can be expressed in a variety of ways, each of which will
be considered below. In terms of the eigenvalues (
)
of the
Hamiltonian matrix it is given by:
 |
(2) |
where
is the Fermi function,
is the chemical
potential for the electrons, kB is Boltzmann's constant, and T is the
temperature of the electrons. Note that below we will often use x to
stand for
.
The eigenvector corresponding to the ntheigenstate is (using Dirac's notation):
 |
(3) |
where i is an atomic site index,
is an atomic orbital index,
and
is an atomic orbital. The eigenvalues and vectors
are found by solving Schrödinger's equation:
 |
(4) |
where
is the
element of the
tight binding Hamiltonian matrix. We define the density of states by:
 |
(5) |
Thus the band energy can be rewritten as:
 |
(6) |
A third way to write the band energy is in terms of the density matrix
which is defined by:
 |
(7) |
In operator notation, the density matrix is given by:
 |
(8) |
The band energy is given by:
 |
(9) |
This last form has the advantage that it allows us to write the band energy
contribution to the atomic forces in a very compact way:
 |
(10) |
Note that this expression for the force assumes that we have included the
electron entropy term, since the electrons have a finite temperature (see
Ref.[18]). The contribution of the
entropy to the free energy is:
 |
(11) |
where
is the entropy density given by
.
Next: Justification of real-space O(N)
Up: A comparison of linear
Previous: Introduction
Dave Bowler
1999-05-17