The development of force fields that accurately describe both the structure
and the dynamics of nucleic acids in condensed phase is an ongoing effort,
The development of the latest versions of the CHARMM and AMBER nucleic aci
ds relied on ab initio as well as on experimental target data for the param
etrization, Here we compare the two latest versions of the AMBER and CHARMM
force field, in their ability to reproduce the ab initio torsional energy
surfaces for selected nucleic acid dihedral angles. A series of model compo
unds is instrumental in this analysis. This illustrates how dissecting the
energetics of the force field with model compounds allows to uncover defici
encies in the force-field, which ma?; or may not be apparent in the simulat
ed properties of the full nucleic acids. The positions of minima, the relat
ive energies and barrier heights are discussed. This type of analysis is pr
oposed as one useful diagnostic criterion, in combination with others. to a
ssess how well balanced are the various contributions to the energetics of
a nucleic acid force field. (C) 2001 Elsevier Science B.V, All rights reser
ved.