------------------------------------------------------------------------------- SEMINAR OF THE LABORATORY FOR COMPUTER DESIGN OF MATERIALS Institute for Computational Sciences and Informatics CSI 929 (http://science.gmu.edu/physics/) ------------------------------------------------------------------------------- Volumetric and Thermal Properties of Asphaltenes from Molecular Dynamics Simulations Mamadou S. Diallo Materials and Process Simulation Center, Beckman Institute California Institute of Technology, Pasadena, CA, 91125 Asphaltenes are complex geomacromolecules operationally defined as the non volatile and polar fractions of crude oil insoluble in aliphatic solvents such as n-heptane. A commonly accepted view in the petroleum chemistry literature is that crude oil asphaltenes form micelles which are stabilized by adsorbed resins kept in solution by aromatics. Two key parametes that control the stability of asphaltene micelles in a crude oil are the ratio of aromatics to saturates and that of resins to asphaltenes. When these ratios decrease, asphaltene micelles will coalesce and form larger aggregates. The precipatation of asphaltene aggreagtes can cause several problems such as reservoir plugging and wettability reversal. The adsorption of asphaltene aggregates at oil-water interfaces has also been shown to cause the steric stabilzation of (W/O) petroleum emulsions. Consequently, the oil industry is in critical need of quantitative tools and thermodynamic data to predict asphaltene aggregation and precipitation as a function of crude oil composition and reservoir temperature and pressure. This presentation will describe a new method of estimation of the thermodynamic properties of asphaltenes. This method combines computer assisted structure elucidation (CASE) with molecular dynamics (MD) simulations. We use quantitative and qualitative structural data as input to a CASE program (SIGNATURE) to generate a sample of ten molecular models of asphaltenes from a Saudi crude oil (Arab Berri).We then use NPT molecular dynamics simulations and molecular mechanics to estimate the molar volume, density, cohesive energy, solubility parameter, enthalpy, thermal expansion coefficient and specific heat at constant pressure of the model asphaltenes structures. We find that the estimated values are in good agreement with the available experimental data. Monday , November 4 1996 5:00 pm Room 206, Science & Tech. I -------------------------------------------------------------------------------