The role of ribonucleic acid (RNA) in biology continues
to grow,
but insight into important aspects of RNA behavior is lacking, such
as dynamic structural ensembles in different environments, how flexibility
is coupled to function, and how function might be modulated by small
molecule binding. In the case of proteins, much progress in these
areas has been made by complementing experiments with atomistic simulations,
but RNA simulation methods and force fields are less mature. It remains
challenging to generate stable RNA simulations, even for small systems
where well-defined, thermostable structures have been established
by experiments. Many different aspects of RNA energetics have been
adjusted in force fields, seeking improvements that are transferable
across a variety of RNA structural motifs. In this work, the role
of weak CH···O interactions is explored, which are
ubiquitous in RNA structure but have received less attention in RNA
force field development. By comparing data extracted from high-resolution
RNA crystal structures to energy profiles from quantum mechanics and
force field calculations, it is shown that CH···O interactions
are overly repulsive in the widely used Amber RNA force fields. A
simple, targeted adjustment of CH···O repulsion that
leaves the remainder of the force field unchanged was developed. Then,
the standard and modified force fields were tested using molecular
dynamics (MD) simulations with explicit water and salt, amassing over
300 μs of data for multiple RNA systems containing important
features such as the presence of loops, base stacking interactions
as well as canonical and noncanonical base pairing. In this work and
others, standard force fields lead to reproducible unfolding of the
NMR-based structures. Including a targeted CH···O adjustment
in an otherwise identical protocol dramatically improves the outcome,
leading to stable simulations for all RNA systems tested.