[General Relativity] Prove that a tensor is a co-tensor

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SUMMARY

This discussion focuses on proving that a co-tensor of rank 2, denoted as ##T_{\mu\nu}##, is derived from a tensor of rank 2, ##T^{\mu\nu}##, by employing a metric to lower the indices, specifically using the equation: $$T_{\mu\nu} = g_{\mu\alpha}g_{\nu\beta}T^{\alpha\beta}$$. Participants clarify the transformation properties of tensors and co-tensors under coordinate changes, emphasizing the role of the Jacobian matrix and metric tensors in these transformations. The conclusion confirms that the transformation of ##T_{\mu\nu}## adheres to the definition of a co-tensor, validating the initial claim.

PREREQUISITES
  • Understanding of tensor notation and operations in General Relativity
  • Familiarity with metric tensors, specifically the role of ##g_{\mu\nu}##
  • Knowledge of coordinate transformations and Jacobian matrices
  • Basic principles of covectors and their transformation properties
NEXT STEPS
  • Study the properties of metric tensors in General Relativity
  • Learn about the transformation laws for tensors and co-tensors
  • Explore the implications of the Jacobian matrix in coordinate transformations
  • Investigate the differences between covectors and tensors of higher ranks
USEFUL FOR

This discussion is beneficial for students and professionals in physics, particularly those studying General Relativity, tensor calculus, and anyone interested in the mathematical foundations of physical theories involving tensors and co-tensors.

mef51
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Hello! I'd appreciate any help or pokes in the right direction.

Homework Statement


Show that a co-tensor of rank 2, ##T_{\mu\nu}##, is obtained from the tensor of rank 2 ##T^{\mu\nu}## by using a metric to lower the indices:
$$T_{\mu\nu} = g_{\mu\alpha}g_{\nu\beta}T^{\alpha\beta}$$

Homework Equations


I know that a vector is a covector if its components transform from one frame to another as:
$$B_\alpha '= \frac {\partial x^\beta}{\partial x'^\alpha } B_\beta$$

The Attempt at a Solution


Analogous to a co-vector, I figure that a tensor of rank 2 is a co-tensor if
$$T_{\alpha\beta} '= \frac {\partial x^\mu}{\partial x'^\alpha } \frac {\partial x^\nu}{\partial x'^\beta } T_{\mu\nu}$$

So I'll start on the right-side and try to simplify it to the left side...
$$
RS = \frac {\partial x^\mu}{\partial x'^\alpha } \frac {\partial x^\nu}{\partial x'^\beta } T_{\mu\nu}
= \frac {\partial x^\mu}{\partial x'^\alpha } \frac {\partial x^\nu}{\partial x'^\beta } g_{\mu\delta} g_{\nu\epsilon} T^{\delta\epsilon}
$$
Now I'll substitute in the Jacobians...
$$
= ({\Lambda^{-1}})^\mu_\alpha ({\Lambda^{-1}})^\nu_\beta g_{\mu\delta} g_{\nu\epsilon} T^{\delta\epsilon}
$$

And I'm not sure where to go from here. I suspect I can contract the jacobians with the metric tensors but I'm not sure how to handle that.

Thanks,
mef
 
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So I think what the problem is asking you is to show that ##T_{\mu\nu}\equiv g_{\mu\alpha}g_{\nu\beta}T^{\alpha\beta}## defined in this way is in fact a co-vector. Is that your interpretation of the problem as well?

In that case, by changing a coordinate system, we should have still ##T_{\mu'\nu'} = g_{\mu'\alpha'}g_{\nu'\beta'}T^{\alpha'\beta'}##. What does the right hand side of this equation look like in terms of un-primed indices?
 
Ok so then we can express the right-side in terms of the unprimed terms using
$$g_{\mu'\alpha'}=(\Lambda^{-1})_{\mu}^{\delta}(\Lambda^{-1})_{\alpha}^{\epsilon}g_{\delta\epsilon}$$
$$g_{\nu'\beta'}=(\Lambda^{-1})_{\nu}^{\eta}(\Lambda^{-1})_{\beta}^{\kappa}g_{\eta\kappa}$$
And we'll get
$$
T_{\mu'\nu'}=g_{\mu'\alpha'}g_{\nu'\beta'}T^{\alpha'\beta'}=(\Lambda^{-1})_{\mu}^{\delta}(\Lambda^{-1})_{\alpha}^{\epsilon}(\Lambda^{-1})_{\nu}^{\eta}(\Lambda^{-1})_{\beta}^{\kappa}g_{\delta\epsilon}g_{\eta\kappa}T^{\alpha'\beta'}=(\Lambda^{-1})_{\mu}^{\delta}(\Lambda^{-1})_{\nu}^{\eta}g_{\delta\epsilon}g_{\eta\kappa}(\Lambda^{-1})_{\alpha}^{\epsilon}(\Lambda^{-1})_{\beta}^{\kappa}T^{\alpha'\beta'}
$$ $$
=(\Lambda^{-1})_{\mu}^{\delta}(\Lambda^{-1})_{\nu}^{\eta}g_{\delta\epsilon}g_{\eta\kappa}T^{\epsilon\kappa}=(\Lambda^{-1})_{\mu}^{\delta}(\Lambda^{-1})_{\nu}^{\eta}T_{\delta\eta}
$$

So we see that ##T_{\mu'\nu'}## transforms as ##T_{\mu'\nu'}=(\Lambda^{-1})_{\mu}^{\delta}(\Lambda^{-1})_{\nu}^{\eta}T_{\delta\eta}## which means that it's a co tensor!
 
Some of your indices should still be primed. Each ##(\Lambda^{-1})^\mu_{~~\nu'}## should have a prime on the bottom index (or else they wouldn't sum over with the T indices in the 3rd and 4th parts of the expression, and they wouldn't match the primped indices on the left hand side of the equation),. Also, usually one would be a bit more general and just leave it in terms of ##\frac{\partial x^\mu}{\partial x^{\nu'}}## so that we can consider more than just Lorentz transformations. But other than that, it looks fine to me.
 
You're right.
My prof has a convention where you only write the primes on the object instead of the indices (so ##T_{\mu\nu}'## instead of ##T_{\mu'\nu'}## and he also defined the transformation ##\Lambda## so that ##\Lambda## has a prime on the top and ##\Lambda^{-1}## has a prime on the bottom:
##\Lambda_{\nu}^{\mu}=\frac{\partial x'^{\mu}}{\partial x^{\nu}}## and ##(\Lambda^{-1})_{\nu}^{\mu}=\frac{\partial x^{\mu}}{\partial x'^{\nu}}##

I prefer priming the indices instead because then you don't have to remember that ##\Lambda^{-1}## has primes on the bottom and vice versa
 
Last edited:

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