Phase field approximation of cohesive fracture models
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We obtain a cohesive fracture model as Γ-limit, as 4915000360&_mathId=si1.gif&_user=111111111&_pii=S0294144915000360&_rdoc=1&_issn=02941449&md5=b65f16ee384160ad4519a8778a986db4" title="Click to view the MathML source">ε→0, of scalar damage models in which the elastic coefficient is computed from the damage variable v   through a function 4915000360&_mathId=si2.gif&_user=111111111&_pii=S0294144915000360&_rdoc=1&_issn=02941449&md5=5594e62deaf47e0d432fc2c78ba413ad" title="Click to view the MathML source">fε of the form 4915000360&_mathId=si3.gif&_user=111111111&_pii=S0294144915000360&_rdoc=1&_issn=02941449&md5=35d435f38bf38d88e670554315bf20e9">View the MathML source4915000360-si3.gif">, with f diverging for v close to the value describing undamaged material. The resulting fracture energy can be determined by solving a one-dimensional vectorial optimal profile problem. It is linear in the opening s at small values of s   and has a finite limit as 4915000360&_mathId=si4.gif&_user=111111111&_pii=S0294144915000360&_rdoc=1&_issn=02941449&md5=85fe607013c8bf0ad1cbdfe191a318a1" title="Click to view the MathML source">s→∞. If in addition the function f is allowed to depend on the parameter ε, for specific choices we recover in the limit Dugdale's and Griffith's fracture models, and models with surface energy density having a power-law growth at small openings.

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