We present an approximation to the total-energy light-binding (TR) met
hod based on use of the kernel polynomial method within a truncated su
bspace. Chebyshev polynomial moments of the Hamiltonian matrix are gen
erated in a stable and efficient manner through recursive matrix-vecto
r multiples. To compute the energy, either the electronic density of s
tates (DOS) or the zero-temperature Fermi function is smeared by convo
lution with the kernel polynomial, with Jackson damping to minimize Gi
bbs oscillations while maintaining the positivity of the DOS. These ar
e shown to give approximate lower and upper bounds, respectively, on t
he exact TB energy, and are averaged to obtain an improved energy esti
mate. The scaling of the computational work is made linear in the numb
er of atoms by truncating the moment computation at a certain range ab
out each atom. Energy derivatives necessary for molecular dynamics are
obtained via a matrix-polynomial derivative relation. The method conv
erges to exact TB as the number of moments and the truncation range ar
e increased. We demonstrate the convergence properties and viability o
f the method for materials simulations in an examination of defects in
silicon. We also discuss the relative importance of truncation range
versus number of moments.