Rate-of-strain tensor in cylindrical coords.

In summary, the conversation revolves around a problem with deriving the rate-of-strain tensor in cylindrical coordinates. The individual is having trouble with some of the terms not being dimensionally consistent and is seeking insight into their error. They are also questioning if they are correctly representing the del operator and taking into account the difference between covariant and contravariant components. The conversation also mentions the use of unit vectors and the transpose of the velocity gradient tensor.
  • #1
JoutlawPhysics
4
0
Hi PF,

I posted this in HW a week ago and got no response. Might be a bit beyond the typical HW forum troller. So, please excuse the double-post.

Homework Statement


I'm trying to derive the rate-of-strain tensor in cylindrical coords, starting with the Christoffel symbols.


Homework Equations



The cylindrical coordinate Christoffel matrices:
\begin{equation}\Gamma^r=\left(
\def\arraystretch{1.5}\begin{array}{ccc}
0&0&0\\
0&-r&0\\
0&0&0
\end{array}\right)
\qquad
\Gamma^\phi=\left(
\def\arraystretch{1.5}\begin{array}{ccc}
0&\dfrac{1}{r}&0\\
\dfrac{1}{r}&0&0\\
0&0&0
\end{array}\right)
\qquad
\Gamma^z=\left(
\def\arraystretch{1.5}\begin{array}{ccc}
0&0&0\\
0&0&0\\
0&0&0
\end{array}\right).
\end{equation}

The gradient of the basis vectors in cylindrical coordinates is
defined in terms of the Christoffel symbols, \[\Gamma^k_{ij}\] such that
\begin{equation}
\nabla_ie_j=\Gamma^k_{ij}e_k.
\end{equation}


The only non-zero terms are
\begin{equation}
\nabla_r e_\phi = \frac{1}{r}e_\phi,\qquad \nabla_\phi e_r =
\frac{1}{r}e_\phi,\qquad \nabla_\phi e_\phi = -r e_r
\end{equation}


The Attempt at a Solution



\begin{eqnarray}
\underline{\underline{\dot{\gamma}}}&=&\nabla\underline{v}= \left(
\def\arraystretch{1.2}\begin{array}{c}
\nabla_r(\underline{v})\\
\nabla_\phi(\underline{v})\\
\nabla_z(\underline{v})
\end{array}\right)=\left(
\def\arraystretch{1.2}\begin{array}{c}
\nabla_r(v_r e_r+v_\phi e_\phi+v_z e_z)\\
\nabla_\phi(v_r e_r+v_\phi e_\phi+v_z e_z)\\
\nabla_z(v_r e_r+v_\phi e_\phi+v_z e_z)
\end{array}\right)\\
&=& \left(
\def\arraystretch{2.2}\begin{array}{c}
(\nabla_rv_r)e_r+\left(\nabla_rv_\phi +v_\phi\dfrac{1}{r}\right)e_\phi+(\nabla_rv_z)e_z\\
(\nabla_\phi v_r-v_\phi r)e_r+\left(\nabla_\phi v_\phi +v_r\dfrac{1}{r}\right )e_\phi +(\nabla_\phi v_z)e_z\\
(\nabla_zv_r)e_r+(\nabla_zv_\phi) e_\phi+(\nabla_zv_z) e_z
\end{array}\right)\nonumber.
\end{eqnarray}

Grouping by basis vectors into individual columns,
\begin{eqnarray}
\underline{\underline{\dot{\gamma}}}
&=&\left(
\def\arraystretch{2.2}\begin{array}{ccc}
\dfrac{\partial v_r }{\partial r}& \dfrac{\partial v_\phi}{\partial r}+\dfrac{v_\phi}{r} & \dfrac{\partial v_z}{\partial r}\\
\dfrac{1}{r}\dfrac{\partial v_r}{\partial\phi}-v_\phi r & \dfrac{1}{r}\dfrac{\partial v_\phi}{\partial\phi}
+\dfrac{v_r}{r} & \dfrac{1}{r}\dfrac{\partial v_z}{\partial\phi} \\
\dfrac{\partial v_r}{\partial z} & \dfrac{\partial v_\phi}{\partial z}
& \dfrac{\partial v_z}{\partial z}
\end{array}\right)
\end{eqnarray}

Symmetrizing,

\begin{eqnarray}
\underline{\underline{\dot{\gamma}}}&=&\frac{\nabla\underline{v}}{2}+\frac{(\nabla\underline{v})^T}{2}\\
&=&\frac{1}{2}\left(
\def\arraystretch{2.2}\begin{array}{ccc}
2\dfrac{\partial v_r }{\partial r}& \dfrac{1}{r}\dfrac{\partial v_r}{\partial\phi}-v_\phi r+\dfrac{\partial v_\phi}{\partial r}+\dfrac{v_\phi}{r} & \dfrac{\partial v_r}{\partial z}+\dfrac{\partial v_z}{\partial r}\\
\dfrac{1}{r}\dfrac{\partial v_r}{\partial\phi}-v_\phi r+\dfrac{\partial v_\phi}{\partial r}+\dfrac{v_\phi}{r} & 2\left(\dfrac{1}{r}\dfrac{\partial v_\phi}{\partial\phi}
+\dfrac{v_r}{r}\right) & \dfrac{\partial v_\phi}{\partial z}+ \dfrac{1}{r}\dfrac{\partial v_z}{\partial\phi} \\
\dfrac{\partial v_r}{\partial z}+\dfrac{\partial v_z}{\partial r} & \dfrac{\partial v_\phi}{\partial z}+\dfrac{1}{r}\dfrac{\partial v_z}{\partial\phi}
& 2\dfrac{\partial v_z}{\partial z}.\nonumber
\end{array}\right)
\end{eqnarray}



To check, I compared this to the rate-of-strain
tensor reported in Batchelor (1967, pg. 602):
\begin{eqnarray}
\underline{\underline{\dot{\gamma}}}&=&\frac{1}{2}\left(
\def\arraystretch{2.2}\begin{array}{ccc}
2\dfrac{\partial v_r }{\partial r}& \dfrac{1}{r}\dfrac{\partial v_r}{\partial\phi}+r\dfrac{\partial}{\partial r}\left(\dfrac{v_\phi}{r}\right) & \dfrac{\partial v_r}{\partial z}+\dfrac{\partial v_z}{\partial r}\\
\dfrac{1}{r}\dfrac{\partial v_r}{\partial\phi}+r\dfrac{\partial}{\partial r}\left(\dfrac{v_\phi}{r}\right) & 2\left(\dfrac{1}{r}\dfrac{\partial v_\phi}{\partial\phi}
+\dfrac{v_r}{r}\right) & \dfrac{\partial v_\phi}{\partial z}+ \dfrac{1}{r}\dfrac{\partial v_z}{\partial\phi} \\
\dfrac{\partial v_r}{\partial z}+\dfrac{\partial v_z}{\partial r} & \dfrac{\partial v_\phi}{\partial z}+\dfrac{1}{r}\dfrac{\partial v_z}{\partial\phi}
& 2\dfrac{\partial v_z}{\partial z}
\end{array}\right)\\
&=&\frac{1}{2}\left(
\def\arraystretch{2.2}\begin{array}{ccc}
2\dfrac{\partial v_r }{\partial r}& \dfrac{1}{r}\dfrac{\partial
v_r}{\partial\phi}+\dfrac{\partial v_\phi}{\partial r}-\dfrac{v_\phi}{r} & \dfrac{\partial v_r}{\partial z}+\dfrac{\partial v_z}{\partial r}\\
\dfrac{1}{r}\dfrac{\partial
v_r}{\partial\phi}+\dfrac{\partial v_\phi}{\partial r}-\dfrac{v_\phi}{r} & 2\left(\dfrac{1}{r}\dfrac{\partial v_\phi}{\partial\phi}
+\dfrac{v_r}{r}\right) & \dfrac{\partial v_\phi}{\partial z}+ \dfrac{1}{r}\dfrac{\partial v_z}{\partial\phi} \\
\dfrac{\partial v_r}{\partial z}+\dfrac{\partial v_z}{\partial r} & \dfrac{\partial v_\phi}{\partial z}+\dfrac{1}{r}\dfrac{\partial v_z}{\partial\phi}
& 2\dfrac{\partial v_z}{\partial z}
\end{array}\right) .\nonumber
\end{eqnarray}

As you can see, the (2,1),(1,2) elements are very different. What am I missing?

Thanks in advance,
Jeff
 
Physics news on Phys.org
  • #2
I'm sorry you are not generating any responses at the moment. Is there any additional information you can share with us? Any new findings?
 
  • #3
Nothing yet. Would still appreciate some insight into my error.
 
  • #4
JoutlawPhysics said:
Nothing yet. Would still appreciate some insight into my error.
Well, for one thing, in your specific tensor components in question, the terms are not dimensionally consistent. The units of each end every term in the rate of deformation tensor must be s-1. This is not the case with one of your vø terms.

Here are some questions:

Are you doing the covariant differentiation correctly, including representing the del operator properly?

Are you taking into account that you might be using the contravariant components of the velocity vector, while Bachelor is using the physical components of the velocity vector (i.e., in terms of the unit vectors, rather than in terms of the coordinate basis vectors).

What about the rate of deformation tensor? Bachelor is expressing the components in terms of the unit vectors. What are you using?

I'm guessing that, when you obtained the velocity gradient tensor, it was in terms of mixed covariant/contravariant components. If that was the case, then you can't simply switch the rows and columns to get the transpose.

Chet
 
Last edited:
  • #5
Chet,

Thanks for the reply. I will follow up on your suggestions. Meanwhile, let me offer one bit of discovery. According to MathWorld, http://mathworld.wolfram.com/CylindricalCoordinates.html, there are two representations of the Christoffel symbols in cylindrical coordinates, one promulgated by Afrken (1985) and one by Misner et al. (1973). I had been using the Arfken representation, since that was what Batchelor presents. However, using the Misner et al. representation does yield the correct form.

My suspicion is that there are features of covariance/contravariance that explain the difference. Perhaps someone with more literacy in these matters can take up the challenge of explaining it. :-)

Thanks,
Jeff
 

1. What is the rate-of-strain tensor in cylindrical coordinates?

The rate-of-strain tensor in cylindrical coordinates is a mathematical representation of the rate at which a fluid is deforming or shearing at a particular point in space. It contains information about the changes in velocity and direction of flow at that point.

2. How is the rate-of-strain tensor calculated in cylindrical coordinates?

The rate-of-strain tensor in cylindrical coordinates is calculated using the velocity gradient tensor, which takes into account the partial derivatives of the velocity components with respect to the cylindrical coordinates. This tensor is then transformed using a rotation matrix to account for the different coordinate system.

3. What are the components of the rate-of-strain tensor in cylindrical coordinates?

The rate-of-strain tensor in cylindrical coordinates has three components: longitudinal strain, circumferential strain, and shear strain. These components represent the deformation of the fluid in the direction of the cylinder axis, around the cylinder, and in the direction perpendicular to the cylinder, respectively.

4. How does the rate-of-strain tensor in cylindrical coordinates relate to the Navier-Stokes equations?

The Navier-Stokes equations, which describe the motion of a fluid, can be derived from the rate-of-strain tensor in cylindrical coordinates. The Navier-Stokes equations take into account the relationship between the rate-of-strain tensor and the stress tensor, which represents the forces acting on the fluid.

5. What are the practical applications of the rate-of-strain tensor in cylindrical coordinates?

The rate-of-strain tensor in cylindrical coordinates is used in various fields of fluid mechanics, such as aerodynamics, hydrodynamics, and rheology. It is also important in the study of blood flow in arteries and in the design of turbines and other rotating machinery. Understanding the rate-of-strain tensor allows scientists and engineers to predict and control the behavior of fluids in these applications.

Similar threads

  • Linear and Abstract Algebra
Replies
5
Views
947
Replies
0
Views
175
  • Linear and Abstract Algebra
Replies
5
Views
944
  • Advanced Physics Homework Help
Replies
1
Views
802
  • Advanced Physics Homework Help
Replies
3
Views
393
  • Classical Physics
Replies
3
Views
1K
  • Special and General Relativity
Replies
1
Views
823
  • Special and General Relativity
Replies
2
Views
753
  • Special and General Relativity
Replies
4
Views
284
  • Advanced Physics Homework Help
Replies
7
Views
1K
Back
Top