Abstract

SUMMARY We incorporate rate- and state-dependent friction in explicit finite difference (FD) simulations of mode II dynamic ruptures in elastic media, using the Mimetic Operators Split-Node (MOSN) method, with adjustable order of spatial accuracy (second-, fourth- or mixed-order accurate), including an option that is fourth-order accurate at the fault discontinuity as well as in the elastic volume. At fault points, the rate and state equations combined with the spatially discretized momentum conservation equations form a coupled system of ordinary differential equations (ODEs) for slip velocity and state variable. As a consequence of the rapid damping of velocity perturbations due to the direct effect, this system exhibits numerical stiffness that is inversely proportional to velocity squared. Approximate solutions to this velocity-state system are achieved by two different implicit schemes: (i) a fourth-order Rosenbrock integration of the full system using multiple substeps and (ii) low order integrations (backward Euler and trapezoidal) of the velocity equation, time-staggered with analytic integration of the state equation under the approximation of constant slip velocity over the time step. In assessing the numerical schemes, we use three test problems: ruptures with frictional resistance controlled by (i) a slip evolution law with strong velocity-weakening behaviour at high slip rates, representing thermal weakening due to flash heating of microscopic asperity contacts, (ii) the classic (low-velocity) slip evolution law and (iii) the classic aging evolution law. A convergence analysis is carried out using reference solutions from a spectral boundary integral equation method (BIEM) (a method restricted to homogeneous media, with nominal spectral accuracy in space and second-order accuracy in time for smooth solutions). Errors are measured by root-mean-square differences of fault-plane time histories (slip, slip rate, traction and state). MOSN shows essentially the same convergence rates as BIEM: second-order convergence for slip and state-variable misfits, with slower (but at least first-order) convergence for slip rates and tractions. For a given grid spacing, fourth-order MOSN is as accurate as BIEM for all variables except slip-rate. MOSN-Rosenbrock nominally has fourth-order temporal accuracy for the fault-plane velocity-state ODE integration (compared to lower-order accuracy for the other two MOSN schemes) and therefore provides an important theoretical benchmark. However, it is sensitive to details of the elastic calculation scheme and occasionally its adaptive substepping performs poorly, leading to large excursions from the reference solution. In contrast, MOSN-trapezoidal is robust and reliable, much easier to implement than MOSN-Rosenbrock, and in all cases achieves precision as good as the latter without recourse to substepping. MOSN-Euler has the same advantages as MOSN-trapezoidal, except that its nominal first-order temporal accuracy ultimately leads to larger errors in slip and state variable compared with the higher-order MOSN schemes at sufficiently small grid spacings and time steps.

Highlights

  • Experimental and theoretical studies of rock friction at high slip speed have the potential to improve our understanding of earthquake rupture mechanics

  • At a given split node, this formulation yields a coupled ordinary differential equations (ODEs) system for slip velocity and state variable that becomes extremely stiff at low slip velocities

  • Convergence rates differ among metrics associated with the fault-plane variables slip, slip rate, shear traction and state variable, respectively

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Summary

Introduction

Experimental and theoretical studies of rock friction at high slip speed (comparable to coseismic slip rates) have the potential to improve our understanding of earthquake rupture mechanics. The Rice (1999) flash-heating equations were tuned by Beeler & Tullis (2003) to fit friction data obtained by Tullis & Goldsby (2003) in high-velocity experiments (up to 0.36 m s−1). To model the transient evolution of fault friction during an earthquake, suitable constitutive models couple flash heating equations to the classic rate- and state-dependent friction (RS) laws introduced by Dieterich (1979) and Ruina (1983) (see Linker & Dieterich 1992). These enhanced rate- and state-dependent friction laws, here called RS-FH laws, model abrupt strength drop at slip rates typical of earthquake rupture propagation (∼1 m s−1), while reducing to the Dieterich–Ruina formulation during slow sliding, so as to model friction during earthquake nucleation, post- and interseismic creep and other low slip-rate processes (e.g. Tse & Rice 1986; Okubo 1989; Lapusta et al 2000; Lapusta & Rice 2003; Rubin & Ampuero 2005)

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