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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 ( $\epsilon^{(n)}$) of the Hamiltonian matrix it is given by:

 \begin{displaymath}U_{band} = 2\sum_n f((\epsilon^{(n)}-\mu)/k_BT)\epsilon^{(n)},
\end{displaymath} (2)

where $f(x)=1/(1+\exp(x))$ is the Fermi function, $\mu$ 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 $(E-\mu)/k_BT$. The eigenvector corresponding to the ntheigenstate is (using Dirac's notation):

 \begin{displaymath}\mid\psi^{(n)}\rangle=\sum_{i\alpha}C^{(n)}_{i\alpha}\mid i\alpha\rangle,
\end{displaymath} (3)

where i is an atomic site index, $\alpha$ is an atomic orbital index, and $\mid i\alpha\rangle$ is an atomic orbital. The eigenvalues and vectors are found by solving Schrödinger's equation:

 \begin{displaymath}\sum_{j\beta}H_{i\alpha,j\beta}C^{(n)}_{j\beta}=\epsilon^{(n)}C^{(n)}_{i\alpha},
\end{displaymath} (4)

where $H_{i\alpha,j\beta}$ is the $(i\alpha,j\beta)$ element of the tight binding Hamiltonian matrix. We define the density of states by:

 \begin{displaymath}n_{total}(E) = \sum_n\delta(E-\epsilon^{(n)}).
\end{displaymath} (5)

Thus the band energy can be rewritten as:

 \begin{displaymath}U_{band} = 2\int{\rm d}E f(x)En_{total}(E).
\end{displaymath} (6)

A third way to write the band energy is in terms of the density matrix which is defined by:

 \begin{displaymath}\rho_{i\alpha,j\beta} = \sum_n C^{(n)}_{i\alpha}f((\epsilon^{(n)}-\mu)/k_BT)
C^{(n)}_{j\beta}.
\end{displaymath} (7)

In operator notation, the density matrix is given by:

 \begin{displaymath}\hat\rho = \sum_n\mid\psi^{(n)}\rangle f((\epsilon^{(n)}-\mu)/k_BT)
\langle\psi^{(n)}\mid.
\end{displaymath} (8)

The band energy is given by:

 \begin{displaymath}U_{band}=2\sum_{i\alpha,j\beta}\rho_{j\beta,i\alpha}H_{i\alpha,j\beta},
\end{displaymath} (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:

 \begin{displaymath}\vec F_{band}^{(k)}=-2\sum_{i\alpha,j\beta}\rho_{j\beta,i\alpha}
{{\partial H_{i\alpha,j\beta}}\over{\partial\vec r_k}}.
\end{displaymath} (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:

 \begin{displaymath}U_{ent} = -2k_BT\int{\rm d}E \sigma(x)n_{total}(E),
\end{displaymath} (11)

where $\sigma(x)$ is the entropy density given by $\sigma(x)=-[f(x)\log f(x)
+(1-f(x))\log(1-f(x))]$.


next up previous
Next: Justification of real-space O(N) Up: A comparison of linear Previous: Introduction
Dave Bowler
1999-05-17