Based on the Hamaker approach, this paper presents a general method to compute the retarded van der Waals (vdW) interaction potential and force between a spherical particle and a cylinder. The effects of the relative dimensions of the cylinder to the sphere were examined by this general method. Firs
Approximations for Calculating van der Waals Interaction Energy between Spherical Particles—A Comparison
✍ Scribed by Suresh N. Thennadil; Luis H. Garcia-Rubio
- Publisher
- Elsevier Science
- Year
- 2001
- Tongue
- English
- Weight
- 93 KB
- Volume
- 243
- Category
- Article
- ISSN
- 0021-9797
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✦ Synopsis
The DLVO theory has been widely used to study the stability of colloidal systems with the van der Waals interactions modeled according to the Hamaker (microscopic) theory. The Hamaker theory, in addition to neglecting many-body interactions, does not account for retardation effects. Retardation effects can be included within the framework of the microscopic theory. For spherical particles, an "exact" expression has been derived by Clayfield et al. Lifshitz (macroscopic) theory, on the other hand, accounts for both manybody and retardation effects but is computationally intensive and requires dielectric data at different frequencies. For spherical particles, it is not practical to use the "exact" expression for van der Waals interaction derived by Langbein; therefore approximations have to be used. Approximate expressions to calculate the van der Waals interaction energy between spheres were considered in terms of accuracy, ease of computation, and required material parameters with the "exact" expression derived by Langbein used as the benchmark. It was found that the "exact" expression using the microscopic theory works as well as the best approximation to the macroscopic theory.
📜 SIMILAR VOLUMES
The van der Waals interaction between perfectly spherical, infinitely hard spheres is well understood. Unfortunately, real powder particles are not infinitely hard and rarely spherical. Those particles that are approximately spherical are often covered in small asperities. It is often believed that