日本地球惑星科学連合2014年大会

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セッション記号 S (固体地球科学) » S-IT 地球内部科学・地球惑星テクトニクス

[S-IT38_30AM1] 地球構成物質のレオロジーと物質移動

2014年4月30日(水) 09:00 〜 10:45 511 (5F)

コンビーナ:*大内 智博(愛媛大学地球深部ダイナミクス研究センター)、桑野 修(独立行政法人海洋研究開発機構)、清水 以知子(東京大学大学院理学系研究科地球惑星科学専攻)、座長:清水 以知子(東京大学大学院理学系研究科地球惑星科学専攻)

10:30 〜 10:45

[SIT38-07] 高速剪断される粉体層の緩和過程と粉体層厚

*桑野 修1中谷 正生2波多野 恭弘2阪口 秀1 (1.海洋研究開発機構、2.東大・地震研)

キーワード:high-velocity friction, granular matter, rheology

A natural fault has the cataclasite core zone, along which shear deformation concentrates. Rheology of these granular matters thus provides us an important insight in considering the nature of friction on faults from a microscopic point of view. In the past two decades, experiments conducted at sub-seismic to seismic slip rates (mm/s to m/s) revealed two remarkable phenomena of high-velocity rock friction; very long critical slip distance (Dc) of the order of 1-10m/s and the considerable weakening due to mechanochemical effects by frictional heating [e.g., Di Toro et al., 2011, Nature]. Recently, Chambon et al.[2006, JGR] conducted friction experiment with very large shear displacement experiment on a thick granular layer, and reported significant slip-weakening behavior active over decimetric slip distances. However, the relation between long Dc observed in a thick granular layer and long Dc in the high-velocity friction is still not clear. Here, we report on laboratory experiments designed to explore transient responses of a thick granular layer following a step change in slip velocity at seismic slip rates. We use simple particle and choose relatively low normal stress to exclude the possible mechanochemical effects caused by frictional heat. We find that friction coefficient and layer thickness show similar response that is symmetry with respect to velocity changes, and Dc is of the order of 10m. It appears that these responses are attributed to dynamics of granular matter. We also report how magnitude of the relaxation and Dc are affected by the layer thickness.