Chebyshev polynomials of the first kind are applied to telescope both
the far-field multipole expansions and the near-field Taylor series ex
pansions used in solving large N-body problems via fast multipole meth
ods. The technique is demonstrated for pairwise-additive, 1/r interpar
ticle potentials in Cartesian coordinates, and a general Mathematica(R
) package is provided to derive the modified expansion coefficients sy
mbolically. Accelerated convergence and more uniform error can be achi
eved without additional computations during runtime. Hence the telesco
ped series require fewer expansion terms for a given accuracy requirem
ent, saving considerable computational expense over conventional fast
multipole implementations. (C) 1995 Academic Press, Inc.