Published July 1, 2003 | Version v1
Journal article

Time-resolved small angle neutron scattering measurements of asphaltene nanoparticle aggregation kinetics in incompatible crude oil mixtures

  • 1. Center for Neutron Research, National Institute of Standards and Technology, Gaithersburg, Maryland 20899 (United States)
  • 2. Corporate Strategic Research, ExxonMobil Research and Engineering Company, Annandale, New Jersey 08801 (United States)

Description

We use time-resolved-small angle neutron scattering to study the kinetics of asphaltene nanoparticle aggregation in incompatible crude oil mixtures. We induce asphaltene aggregation by mixing asphaltene-rich Syrian crude oil (SACO) with a paraffinic British crude oil and observe the scattered neutron intensity, I, as a function of wave number, q, over times, t, ranging from twenty minutes to about a week. We observe a growth in I at low q as the nanoscale asphaltenes agglomerate into microscale aggregates and interpret this growth as an increase in surface scattering from the aggregates. We fit I(q,t) to an empirical model and measure the growth in the power-law exponent, α, associated with the low-q logarithmic slope of I(q). We define a time, τα, associated with the first appearance of the aggregates when α>3; τα increases as a function of the volume fraction, φm, of SACO in the mixture. The surface scattering intensity initially increases and then saturates at long times when the aggregate structures no longer evolve at the length scales we probe. Based on this saturation, we define a time scale, τI, which is larger than τα but has essentially the same dependence on φm. We interpret τα(φm) and τI(φm) in terms of a simple aggregation model based on diffusion-limited kinetics and a repulsive potential barrier that models the effective solvent quality

Additional details

Identifiers

Publishing Information

Journal Title
Journal of Chemical Physics
Journal Volume
119
Journal Issue
1
Journal Page Range
p. 565-571
ISSN
0021-9606
CODEN
JCPSA6

Optional Information

Notes
(c) 2003 American Institute of Physics.