We present a computational investigation of the sulfuric
acid,
glycine, serine, ammonia, and water system to understand if this system
can form prenucleation clusters, which are precursors to larger aerosols
in the atmosphere. We have performed a comprehensive configurational
search of all possible clusters in this system, starting with the
four different monomers and zero to five waters. Accurate Gibbs free
energies of formation have been calculated with the DLPNO-CCSD(T)/complete
basis set (CBS) method on ωb97xd/6-31++G** geometries. For the
dry dimers of sulfuric acid, the weakest base, serine, is found to
form the most stable complex, which is a consequence of the strong
di-ionic complex formed between the bisulfate ion and the protonated
serine cation. For the dry dimers without sulfuric acid, the glycine–serine
complex is more stable than the glycine–ammonia or serine–ammonia
complexes, stemming from the detailed structure and not related to
base strength. For the larger complexes, sulfuric acid deprotonates
and the proton is shifted to glycine, serine, or ammonia. The two
amino acids and ammonia are almost interchangeable and there is no
easy way to predict which molecule will be protonated without the
calculated results. Assuming reasonable starting concentrations and
a closed system of sulfuric acid, glycine, serine, ammonia, and five
waters, we predict the concentrations of all possible complexes at
two temperatures spanning the troposphere. The most negative ΔG° values are a function of the detailed molecular
interactions of these clusters. These details are more important than
the base strength of ammonia, glycine, and serine.