Abstract
Frictional motion is mediated by rapidly propagating ruptures that detach the ensemble of contacts forming the frictional interface between contacting bodies1,2,3,4,5,6,7. These ruptures are similar to shear cracks. When this process takes place in natural faults, these rapid ruptures are essentially earthquakes8,9. Although fracture mechanics describe the rapid motion of these singular objects, the nucleation process that creates them is not understood10,11,12,13,14,15,16,17,18,19. Here we fully describe the nucleation process by extending fracture mechanics to explicitly incorporate finite interface widths (which are generally ignored20,21). We show, experimentally and theoretically, that slow steady creep ensues at a well-defined stress threshold. Moreover, as slowly creeping patches approach the interface width, a topological transition takes place in which these creeping patches smoothly transition to the rapid fracture that is described by classical fracture mechanics22,23,24,25,26. Apart from its relevance to fracture and material strength, this new picture of rupture nucleation dynamics is directly relevant to earthquake nucleation dynamics; slow, aseismic rupture must always precede rapid seismic rupture (so long as the initial defect in the interface is localized in both spatial dimensions). The theory may provide a new framework for understanding how and when earthquakes nucleate.
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Data availability
The raw data (camera recordings and strain gauge measurements) for all events analysed in this paper can be accessed directly at https://doi.org/10.4121/12631fa1-4fed-440d-acf3-676b97862034. More information and other findings of this study are available from the corresponding author upon request. Source data are provided with this paper.
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Acknowledgements
J.F. and S.G. acknowledge the support of the Israel Science Foundation (grant no. 416/23).
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S.G. performed the experimental measurements. S.G. and J.F. contributed to the data analysis and experimental design. M.A-B. led the derivation of the theory, with contributions from the other authors. D.S.K. performed all of the numerical work. All authors contributed to the writing of the paper and overall analysis.
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Extended data figures and tables
Extended Data Fig. 1 The stress intensity factor K of an arrested rupture is determined by strain gage measurements.
a. Strain gage measurements (symbols) of the measured stress changes, Δσxx, excited by a rupture that arrested at point xarrest, as a function of x − xarrest. Fitted LEFM predictions (see Eq. (6)) (lines) compare well with the strain gage measurements, when K is the sole fitting parameter. Shown are 3 different events, each with a different value of varr, the rupture velocity immediately prior to rupture arrest at imposed barriers. b. The initial ‘pre-stress’ data, \({\sigma }_{xy}^{pre}\), measured at the nucleation site in a single sequence of 30 induced nucleation events. Red symbols are events in which the previous arrested rupture triggered a nucleation event. In these cases \({\sigma }_{xy}^{pre} \sim 0\). Blue symbols denote \({\sigma }_{xy}^{pre}\) for events in which the previous arrested rupture did not trigger a nucleation event. These finite pre-stresses need to be accounted for to correctly determine the shear stress, τ, at the nucleation site.
Extended Data Fig. 2 The real contact area and rupture front positions are determined optically.
(a,b) Imaging system - the entire contact interface was illuminated by a sheet of incoherent light directed at an incident angle 28° beyond the critical angle (41.8°) for total internal reflection from PMMA to air. Light impinging on non-contacting regions of the interface was reflected away from the interface. Incident light was only transmitted through the interface at the points of contact. The transmitted light was recorded at 580000 frames/sec by a fast camera (Phantom V711) at an x × z spatial resolution of 1280 × 8 pixels. c. Close up of a non-normalized image. The light intensity19 at each point yields a rough topographic image of the contacting points (each x, z pixel is mapped to an area of 156 × 688 μm that contains about 1000 contacts). d. Temporal sequence of normalized contact areas, \({\mathcal{A}}(x,z,t)/{{\mathcal{A}}}_{0}(x,z)\), in which the motion of the (effectively 1D) rupture front propagating at approximately 1000m/s (0.8CR) is evident. The x, z dimensions are as in c. Intervals between frames are 3.4 μs.
Extended Data Fig. 3 In a spatially confined interface, the rupture area and perimeter are independent entities, until the topological transition to a 1D rupture front.
a. Schematic representation of the generic problem of failure nucleation in a confined geometry. b. Schematic evolution of the rupture: the perimeter P(t) of the crack front as function of its area A(t).
Extended Data Fig. 4 The stress released by a nucleation patch changes its character from ‘penny crack’ scaling to ‘through crack’ scaling with the distance from the patch.
Numerical results from FE simulations. a. Normalized excess potential energy as a function of crack radius R. The dashed line is the least squares cubic fit: ΔΩ/Ω0 = 3.25(R/W)3. b. Tensile stress σyy difference along a line perpendicular to the crack plane starting from its center, for two different R/W ratios. Trends, corresponding to the scaling derived in Eq. (15), are shown in dashed (far field) and dotted (near field) gray lines.
Extended Data Fig. 5 As the mapped ‘1D’ crack length approaches W, a topological transition from the ‘penny-like’ to ‘through-crack’ failure regimes occurs.
a. Schematic view of 3D rupture propagation in a confined geometry. The rupture is characterized by its perimeter P(t) and the enclosed area, A(t). These are mapped to the 2D configuration characterized by a straight crack front of length ℓ(t). b. The generic behavior of the perimeter P(t) in the original problem as function of the crack length ℓ(t) in the mapped configuration.
Extended Data Fig. 6 The shape function, β(ℓ), characterizing self-similar nucleation patches is particularly simple during the nucleation phase, until the topological transition to 1D rupture occurs at ℓ*.
a. The shape function β(ℓ) for a self-similar growth of a penny crack shown in the inset. Note that, in this case, β = π/2 for ℓ < ℓ* = W, where ℓ* is the value of ℓ at which the topological transition takes place. b. Mode I (g1(v)) and mode II (g2(v)) solutions of self-similar Broberg problems23. Here, plane stress conditions are imposed so that the dilatational (cd) and shear (cs) wave speeds are related by \({c}_{d}=\sqrt{2/(1-\rho )}{c}_{s}\), where ρ = 1/3 is the Poisson ratio.
Extended Data Fig. 7 The transition from slow nucleation to rapid ‘1D’ dynamics for a self-similar nucleation patch.
The dynamics of tensile (mode I) and shear (mode II) rupture fronts corresponding to the case depicted in Extended Data Fig. 6 with LG ≈ 0.62W.
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Gvirtzman, S., Kammer, D.S., Adda-Bedia, M. et al. How frictional ruptures and earthquakes nucleate and evolve. Nature 637, 369–374 (2025). https://doi.org/10.1038/s41586-024-08287-y
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DOI: https://doi.org/10.1038/s41586-024-08287-y
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