Abstract

Abstract. The local topographic slope of the accretionary prism is often used together with the critical taper theory to determine the effective friction on subduction megathrust. In this context, extremely small topographic slopes associated with extremely low effective basal friction (μ≤0.05) can be interpreted either as seismically locked portions of megathrust, which deforms episodically at dynamic slip rates or as a viscously creeping décollement. Existing mechanical models of the long-term evolution of accretionary prism, sandbox models, and numerical simulations alike, generally do not account for heat conservation nor for temperature-dependent rheological transitions. Here, we solve for advection–diffusion of heat with imposed constant heat flow at the base of the model domain. This allows the temperature to increase with burial and therefore to capture how the brittle–ductile transition and dehydration reactions within the décollement affect the dynamic of the accretionary prism and its topography. We investigate the effect of basal heat flow, shear heating, thermal blanketing by sediments, and the thickness of the incoming sediments. We find that while reduction of the friction during dewatering reactions results as expected in a flat segment often in the forearc, the brittle–ductile transition results unexpectedly in a local increase of topographic slope by decreasing internal friction. We show that this counterintuitive backproduct of the numerical simulation can be explained by the onset of internal ductile deformation in between the active thrusts. Our models, therefore, imply significant viscous deformation of sediments above a brittle décollement, at geological rates, and we discuss its consequences in terms of interpretation of coupling ratios at subduction megathrust. We also find that, with increasing burial and ductile deformation, the internal brittle deformation tends to be accommodated by backthrusts until the basal temperature becomes sufficient to form a viscous channel, parallel to the décollement, which serves as the root to a major splay fault and its backthrust and delimits a region with a small topographic slope. Morphologic resemblances of the brittle–ductile and ductile segments with forearc high and forearc basins of accretionary active margins, respectively, allow us to propose an alternative metamorphic origin of the forearc crust in this context.

Highlights

  • Several studies have suggested a link between the morphology of forearc wedges and the seismic behavior of megathrusts, showing a correlation between large subduction earthquakes and forearc basins or deep-sea terraces (Wells et al, 2003) or with negative free-air gravity anomalies (Song and Simons, 2003; Wells et al, 2003).Forearc wedges are to the first order well described by the critical taper theory (CTT) (Davis et al, 1983; Dahlen et al, 1984)

  • Using the location of the splay fault in warm, compressional accretionary contexts like South Sumatra (Fig. 10b) and Lesser Antilles (Fig. 10c), we propose that what is typically interpreted as attenuated continental or arc crust with Vp>=5 could well mark the location of the brittle–ductile transition According to our models, along with accretionary prisms of little seismic activity, the forearc basin should correlate with the fully viscous domain at least along high sedimentation rate and high thermal gradient compressive accretionary margins (Fig. 9a)

  • – brittle décollement and viscous internal deformation of fault-bounded blocks, where the topographic slope is in excess compared to the CTT and these large slopes should not be interpreted as the down-dip limit of the seismogenic zone;

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Summary

Introduction

Forearc wedges are to the first order well described by the critical taper theory (CTT) (Davis et al, 1983; Dahlen et al, 1984) This theory assumes that wedges are built by accretion of material equivalent to sand pushed by a moving bulldozer over a frictional basal décollement. This theory has been very successful in describing the equilibrium morphology of wedges in response to accretion and as a function of its effective internal and basal frictional strength (Davis et al, 1983; Dahlen et al, 1984). Prograde metamorphic reactions that affect clay minerals release water in the system, which is suspected to raise fluid pressure and diminish effective friction Clay contents, their nature, and their evolution during accretion may affect the effective friction of the décollement as a function of temperature history

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