Counterions under a Surface-Adsorbed Cationic Surfactant Monolayer: Structure and Thermodynamics

Eli Sloutskin, Lilach Tamam, Zvi Sapir, Benjamin M. Ocko, Colin D. Bain, Ivan Kuzmenko, Thomas Gog, Moshe Deutsch

Research output: Contribution to journalArticlepeer-review

7 Scopus citations

Abstract

The surface adsorption of ionic surfactants is fundamental for many widespread phenomena in life sciences and for a wide range of technological applications. However, direct atomic-resolution structural experimental studies of noncrystalline surface-adsorbed films are scarce. Thus, even the most central physical aspects of these films, such as their charge density, remain uncertain. Consequently, theoretical models based on contradicting assumptions as for the surface films' ionization are widely used for the description and prediction of surface thermodynamics. We employ X-ray reflectivity to obtain the Ångström-scale surface-normal structure of surface-adsorbed films of the cationic surfactant cetyltrimethylammonium bromide (CTAB) in aqueous solutions at several different temperatures and concentrations. In conjunction with published neutron reflectivity data, we determine the surface-normal charge distribution due to the dissociated surfactants' headgroups. The distribution appears to be inconsistent with the Gouy-Chapman model yet consistent with a compact Stern layer model of condensed counterions. The experimental surfactant adsorption thermodynamics conforms well to classical, Langmuir and Kralchevsky, adsorption models. Furthermore, the Kralchevsky model correctly reproduces the observed condensation of counterions, allowing the values of the adsorption parameters to be resolved, based on the combination of the present data and the published surface tension measurements.

Original languageEnglish
Pages (from-to)12356-12366
Number of pages11
JournalLangmuir
Volume38
Issue number40
DOIs
StatePublished - 11 Oct 2022

Bibliographical note

Publisher Copyright:
© 2022 American Chemical Society. All rights reserved.

Funding

We thank R. Netz and C. Fleck for important discussions. This research is supported by the Israel Science Foundation (grant no. 2205/21). Beamtime at beamlines X22B at NSLS and at 9ID at APS is gratefully acknowledged. BNL is supported by U.S. DOE Contract DE-AC02-98CH10886. Use of the Advanced Photon Source at Argonne National Laboratory was supported by the U.S. Department of Energy, Office of Science, Office of Basic Energy Sciences (contract no. DE-AC02-06CH11357).

FundersFunder number
U.S. Department of EnergyDE-AC02-98CH10886
Office of Science
Basic Energy SciencesDE-AC02-06CH11357
Israel Science Foundation2205/21

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