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Instability in dynamic fracture and the failure of the classical theory of cracks

Understanding crack formation is important for improving the mechanical performance of materials. A new theory is now presented for the description of cracks propagating at high speeds, with elastic nonlinearity as the underlying principle. Cracks, the major vehicle for material failure 1 , undergo...

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Bibliographic Details
Published in:Nature physics 2017-12, Vol.13 (12), p.1186-1190
Main Authors: Chen, Chih-Hung, Bouchbinder, Eran, Karma, Alain
Format: Article
Language:English
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Summary:Understanding crack formation is important for improving the mechanical performance of materials. A new theory is now presented for the description of cracks propagating at high speeds, with elastic nonlinearity as the underlying principle. Cracks, the major vehicle for material failure 1 , undergo a micro-branching instability at ∼40% of their sonic limiting velocity in three dimensions 2 , 3 , 4 , 5 , 6 . Recent experiments showed that in thin systems cracks accelerate to nearly their limiting velocity without micro-branching, until undergoing an oscillatory instability 7 , 8 . Despite their fundamental importance, these dynamic instabilities are not explained by the classical theory of cracks 1 , which is based on linear elasticity and an extraneous local symmetry criterion to predict crack paths 9 . We develop a two-dimensional theory for predicting arbitrary paths of ultrahigh-speed cracks, which incorporates elastic nonlinearity without extraneous criteria. We show that cracks undergo an oscillatory instability controlled by small-scale, near crack-tip, elastic nonlinearity. This instability occurs above an ultrahigh critical velocity and features an intrinsic wavelength proportional to the ratio of the fracture energy to the elastic modulus, in quantitative agreement with experiments. This ratio emerges as a fundamental scaling length assumed to play no role in the classical theory of cracks, but shown here to strongly influence crack dynamics.
ISSN:1745-2473
1745-2481
DOI:10.1038/nphys4237