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Energy Modeling of Competition Between Tubular and Platy Morphologies of Chrysotile and Halloysite Layers

Published online by Cambridge University Press:  01 January 2024

Andrei A. Krasilin*
Affiliation:
Ioffe Institute, 26 Politekhnicheskaya st., St. Petersburg 194021, Russia
*
*E-mail address of corresponding author: ikrasilin@mail.ioffe.ru
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Abstract

The present study considered the problem of halloysite nanoscroll synthesis by energy modeling of the formation of chrysotile and halloysite particles. The main aim of the study was to reveal an energy preference between scrolled and platy morphologies of the particles. Both hydrosilicates possess the ability to scroll spontaneously but relatively facile hydrothermal synthesis of the nanoscrolls is available only to the former, whereas halloysite forms mainly plates under the same conditions. This issue was investigated by a phenomenological energy model, taking into account: (1) strain energy due to the size difference between metal oxide and silica sheets; (2) surface-energy difference on the opposite sides of the layer; and (3) adhesion energy. Calculations showed that the halloysite layer had a significant scrolling potential due to the first energy component, but the surface-energy difference acted in the opposite direction and tried to unbend the layer. In contrast, these two actions were co-directional in chrysotile layers. In both cases, the formation of multi-layered plates became more energy favorable when the specific surface energy of the edges decreased. In the range 0.5–3 J/m2 for the specific surface energy, only halloysite layers showed an energy preference for platy particles over nanoscrolls, especially at small layer sizes. Certain processes, such as hydration, could reduce the corresponding specific surface energy value and, as a result, could stabilize the platy morphology of halloysite at the earliest stages of particle growth under hydrothermal conditions.

Information

Type
Original Paper
Copyright
Copyright © Clay Minerals Society 2020
Figure 0

Fig. 1. Calculation concepts. a Covalent bonding of two different sheets yielded chrysotile and halloysite layers. Sheet structures were adopted from Saalfeld and Wedde (1974), Desgranges et al. (1996), Churakov et al. (2004), and Roveri et al. (2006) using VESTA software (Momma and Izumi 2011). b Structural parameters of the layers. c Scrolling and stacking of layers

Figure 1

Table 1. Structural parameters of the energy model for chrysotile and halloysite layers

Figure 2

Fig. 2. Preferred size parameters (inner and outer radii of curvature) and energy effect of scrolling (∆E/@) of a chrysotile and b halloysite layers. The position of the principal energy minimum is marked by a vertical line. Influence of Young’s modulus on c chrysotile and d halloysite preferred radii of curvature. Influence of the specific surface energy value of the octahedral sheet (σoct, which is equal to σout or σin) on e chrysotile and f halloysite preferred radii of curvature

Figure 3

Fig. 3. Energy effect of scrolling (∆E/@), formation of a multi-layered plate (∆E/=), and the difference curve

Figure 4

Fig. 4. Energy effect of scrolling (∆E/@) and formation of a multi-layered plate (∆E/=) vs. the number of layers (n, k) in the case of halloysite with σe = 0.5 J/m2. The points denoting the energy effect of plate formation are joined by a dashed line for the sake of clarity. The insets show the approximate geometry of the cross sections of the particles