Strain (materials science)
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- This article is about the deformation of materials. For other meanings, see strain.
In any branch of science dealing with materials and their behaviour, strain is the geometrical expression of deformation caused by the action of stress on a physical body. Strain therefore expresses itself as a change in size and/or shape. In the case of geological action of the earth, if the release of stress through strain in rocks is sufficiently large, earthquakes may occur.
If strain is equal over all parts of a body, it is referred to as homogeneous strain; otherwise, it is inhomogeneous strain. In its most general form, the strain is a symmetric tensor.
Quantifying strain
Given that strain results in the deformation of a body, it can be measured by calculating the change in length of a line or by the change in angle between two lines (where these lines are theoretical constructs within the deformed body). The change in length of a line is termed the stretch or absolute strain, and may be written as <math>\delta \ell</math>. Then the (relative) strain, <math>\epsilon \;</math>, is given by
- <math>\epsilon = \frac {\delta \ell}{\ell_0}</math>
where <math>\ell_o</math> is the original length of the material and <math>\delta \ell</math> is the extension. The extension is positive if the material has gained length (in tension), and negative if it has reduced length (in compression). The sign of the stretch is then passed on to the strain.
Strain has no units of measure because in the formula the units of length are cancelled. Dimensions of metres/metre or inches/inch are sometimes used for convenience, but generally units are left off and the strain sometimes is given as a percentage.
Engineering strain vs. true strain
The above definition (known technically as engineering strain) is not linear, in that strains cannot be totalled. Imagine that a body is deformed twice, first by <math>\delta \ell_1</math> and then by <math>\delta \ell_2</math> (cumulative deformation). The final strain
- <math>\epsilon = \frac{\delta \ell_1 + \delta \ell_2}{\ell_0}</math>
is slightly different from the sum of the strains:
- <math>\epsilon_1 = \frac{\delta \ell_1}{\ell_0}</math>
and
- <math>\epsilon_2 = \frac{\delta \ell_2}{\ell_0 + \delta \ell_1}</math>
As long as <math>\delta \ell_1 \ll \ell_0</math>, it is possible to write:
- <math>\epsilon_2 \simeq \frac{\delta \ell_2}{\ell_0}</math>
and thus
- <math>\epsilon \;= \epsilon_1 \; + \epsilon_2 \;</math>
True strain, however, can be totalled. This is defined by:
- <math>\exp(\epsilon) = \frac{d\ell}{\ell}</math>
and thus
- <math>\epsilon = \ln \left (\frac{\ell}{\ell_0} \right )</math>
The engineering strain formula is the series expansion of the true strain formula.