Magnetic vs. non-magnetic colloids – A comparative adsorption study to quantify the effect of dye-induced aggregation on the binding affinity of an organic dye
[Display omitted] Due to attractive magnetic forces, magnetic particles (MPs) can exhibit colloidal instability upon molecular adsorption. Thus, by comparing the dye adsorption isotherms of MPs and non-magnetic particles of the same size, shape and functional group it should be possible to character...
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Published in: | Journal of colloid and interface science Vol. 481; pp. 20 - 27 |
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Main Authors: | , , , |
Format: | Journal Article |
Language: | English |
Published: |
United States
Elsevier Inc
01-11-2016
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Subjects: | |
Online Access: | Get full text |
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Summary: | [Display omitted]
Due to attractive magnetic forces, magnetic particles (MPs) can exhibit colloidal instability upon molecular adsorption. Thus, by comparing the dye adsorption isotherms of MPs and non-magnetic particles of the same size, shape and functional group it should be possible to characterize the influence of magnetic attraction on MP aggregation.
For a range of particle densities, a comparative adsorption study of malachite green (MG+) onto magnetic and non-magnetic colloids was carried out using a combination of a separation technique coupled with UV–vis spectroscopy, optical microscopy, and polarization dependent second harmonic generation (SHG) spectroscopy.
Significant MP aggregation occurs in aqueous solution due to MG+ adsorption. This alters the adsorption isotherm and challenges the determination of the adsorption equilibrium constant, Kads. The dye-induced aggregation is directly related to the MG+ concentration, [MG+]. A modified Langmuir equation, which incorporates loss of surface sites due to this aggregation, accurately describes the resulting adsorption isotherms. The Kads of 1.1 (±0.3)×107 and a loss of maximum MP surface capacity of 2.8 (±0.7)×103M−1 per [MG+] has been obtained. Additionally, SHG has been established as an effective tool to detect aggregation in nanoparticles. |
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Bibliography: | ObjectType-Article-1 SourceType-Scholarly Journals-1 ObjectType-Feature-2 content type line 23 |
ISSN: | 0021-9797 1095-7103 |
DOI: | 10.1016/j.jcis.2016.07.038 |