The w:Polar decomposition theorem states that any second order tensor whose determinant is positive can be decomposed uniquely into a symmetric part and an orthogonal part.
In continuum mechanics, the deformation gradient is such a tensor because . Therefore we can write
where is an orthogonal tensor () and are symmetric tensors ( and ) called the right stretch tensor and the left stretch tensor, respectively. This decomposition is called the polar decomposition of .
Recall that the right Cauchy-Green deformation tensor is defined as
Clearly this is a symmetric tensor. From the polar decomposition of we have
If you know then you can calculate and hence using .
If you want to find given you will need to take the square root of . How does one do that?
We use what is called the spectral decomposition or eigenprojection of . The spectral decomposition involves expressing in terms of its eigenvalues and eigenvectors. The tensor product of the eigenvectors acts as a basis while the eigenvalues give the magnitude of the projection.
where are the principal values (eigenvalues) of and are the principal directions (eigenvectors) of .
Since the basis does not change, we then have
Therefore the λi can be interpreted as principal stretches and the vectors are the directions of the principal stretches.
Let us assume that the motion is given by
The adjacent figure shows how a unit square subjected to this motion evolves over time.
The deformation gradient is given by
At t = 1 at the position we have
You can calculate the deformation gradient at other points in a similar manner.
To compute we have to find the eigenvalues and eigenvectors of . The eigenvalue problem is
To find the eigenvalues we solve the characteristic equation
Plugging in the numbers, we get
This equation has two solutions
Taking the square roots we get the values of the principal stretches
To compute the eigenvectors we plug into the eigenvalues into the eigenvalue problem to get
Because this system of equations is not linearly independent, we need another equation to solve this system of equations for and . This problem is eliminated by using the following equation (which implies that is a unit vector)
Solving, we get
We can do the same thing for the other eigenvector to get
We usually don't see any problem to calculate at this point and go straight to the right stretch tensor.
The right stretch tensor is given by
We can invert this matrix to get
We can now find the rotation matrix by using th relation
In matrix form,
You can check whether this matrix is orthogonal by seeing whether .
You thus get the polar decomposition of . In an actual calculation you have to be careful about floating point errors. Otherwise you might not get a matrix that is orthogonal.