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The Role of Grain Boundaries in Low-Temperature Plasticity of Olivine Revealed by Nanoindentation

Accepted version
Peer-reviewed

Type

Article

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Abstract

Rheological properties of olivine influence large-scale, long-term deformation processes on rocky planets. Studies on the deformation of olivine at low temperatures and high stresses have emphasized the importance of a grain-size effect impacting yield stress. Laboratory studies indicate that aggregates with finer grains are stronger than those with coarser grains. However, the specific interactions between intracrystalline defects and grain boundaries leading to this effect in olivine remain unresolved. In this study, to directly observe and quantify the mechanical properties of olivine grain boundaries, we conduct nanoindentation tests on well characterized bicrystals. Specifically, we perform room temperature spherical and Berkovich nanoindentation tests on a subgrain boundary (13°, [100]/(016)) and a high-angle grain boundary (60°, [100]/(011)). These tests reveal that plasticity is easier to initiate if the high-angle grain boundary is within the deformation volume, whereas the subgrain boundary does not impact the initiation of plasticity. Additionally, the high-angle grain boundary acts as a barrier to slip transmission, whereas the subgrain boundary does not interact with dislocations in a measurable manner. We suggest that the distribution of grain-boundary types in olivine-rich rocks might play a role in generating local differences during deformation.

Description

Keywords

37 Earth Sciences, 3705 Geology, 3706 Geophysics

Journal Title

Journal of Geophysical Research: Solid Earth

Conference Name

Journal ISSN

2169-9313
2169-9356

Volume Title

Publisher

American Geophysical Union
Sponsorship
MRC (MR/V021788/1)
DA is grateful to the UK National Environmental Research Council, and the Oxford Doctoral Training Partnership for DPhil studentship and funding [grant number NE/L002612/1]. LH, KM, and AW acknowledge funding from UK National Environmental Research Council, via the NERC Standard Grant [grant number NE/S00162X/1]. LH acknowledges funding from the National Science Foundation [grant number NSF-EAR Grant 2022433]. DW acknowledges the support of a UKRI Future Leaders Fellowship [grant number NE/M000966/1], and the Netherlands Organisation for Scientific Research, User Support Programme Space Research [grant number ALWGO.2018.038].