Some trouble with relativistic notations

In summary, the conversation discusses solving a problem related to the Lagrangian and the energy-momentum tensor. The conversation includes equations and attempts at solutions, with a particular focus on the derivatives and indices of the tensor. The use of the metric tensor is also mentioned.
  • #1
Amentia
110
5
Hello, I am trying to solve a problem and I have trouble with almost every part of it.

Homework Statement


For the Lagrangian
[tex]L=-\frac{1}{4}F_{\mu\nu}F^{\mu\nu}[/tex]
show that
[tex]\Pi^{\sigma\rho} = \frac{\partial L}{\partial(\partial_{\sigma}A_{\rho})}=-F^{\sigma\rho}[/tex]
Hence show that the energy-momentum tensor
[tex]T_{\nu}^{\mu} = \Pi^{\mu\sigma}\partial_{\nu}A_{\sigma}-\delta_{\nu}^{\mu}L[/tex]
can be written as
[tex]T^{\mu\nu} = -F^{\mu\sigma}\partial^{\nu}A_{\sigma}+\frac{1}{4}g^{\mu\nu}F^{\alpha\beta}F_{\alpha\beta}[/tex]
We symmetrize the tensor by adding
[tex]\partial_{\lambda}X^{\lambda\mu\nu} \text{ with } X^{\lambda\mu\nu}=F^{\mu\lambda}A^{\nu}[/tex]
Show that the new tensor is:
[tex]\hat{T}^{\mu\nu}=F^{\mu\sigma}F_{\sigma}^{\nu} + \frac{1}{4}g^{\mu\nu}F^{\alpha\beta}F_{\alpha\beta}[/tex]

Homework Equations


[tex]F_{\alpha\beta} = \partial_{\alpha}A_{\beta}-\partial_{\beta}A_{\alpha}[/tex]
[tex]F^{\alpha\beta} = \partial^{\alpha}A^{\beta}-\partial^{\beta}A^{\alpha}[/tex]

The Attempt at a Solution


[tex]\Pi^{\sigma\rho} = \frac{\partial L}{\partial(\partial_{\sigma}A_{\rho})}[/tex]
[tex]\Pi^{\sigma\rho}=-\frac{1}{4}\frac{\partial}{\partial(\partial_{\sigma}A_{\rho})}\left([\partial_{\alpha}A_{\beta}-\partial_{\beta}A_{\alpha}]F^{\alpha\beta}\right)[/tex]
[tex]\Pi^{\sigma\rho}=-\frac{1}{4}\left([\frac{\partial(\partial_{\alpha}A_{\beta})}{\partial(\partial_{\sigma}A_{\rho})}-\frac{\partial(\partial_{\beta}A_{\alpha})}{\partial(\partial_{\sigma}A_{\rho})}]F^{\alpha\beta}\right)[/tex]
[tex]\Pi^{\sigma\rho}=-\frac{1}{4}\left(\delta_{\sigma}^{\alpha}\delta_{\rho}^{\beta}-\delta_{\sigma}^{\beta}\delta_{\rho}^{\alpha}\right)F^{\alpha\beta}
[/tex]
[tex]\Pi^{\sigma\rho}=-\frac{1}{4}(F^{\sigma\rho}-F^{\rho\sigma})[/tex]
[tex]\Pi^{\sigma\rho}=-\frac{1}{4}(F^{\sigma\rho}+F^{\sigma\rho})[/tex]
[tex]\Pi^{\sigma\rho}=-\frac{1}{2}F^{\sigma\rho}[/tex]

So I don't know where the missing factor 2 should appear in my result. I am not used to taking such derivatives but it seems obvious to me that it must give a delta function because only one of the terms does not vanish. And I don't see where is my mistake. Unless the tensor with upper indices is not a constant for this operator of derivation.

Next, let's assume I have the correct result...
[tex]T_{\nu}^{\mu} = \Pi^{\mu\sigma}\partial_{\nu}A_{\sigma}-\delta_{\nu}^{\mu}L[/tex]
[tex]T_{\nu}^{\mu} = -F^{\mu\sigma}\partial_{\nu}A_{\sigma}+\frac{1}{4}\delta_{\nu}^{\mu}F_{\alpha\beta}F^{\alpha\beta}[/tex]

Here it looks close to the expected result but I don't understand how the indices are rised. And what is the point of moving nu from a lower index to the top?

For the last calculation, one term is the same, so I work the other one:
[tex] -F^{\mu\sigma}\partial^{\nu}A_{\sigma}+\partial_{\lambda}(F^{\mu\lambda}A^{\nu})=-F^{\mu\sigma}\partial^{\nu}A_{\sigma}+\partial_{\lambda}(F^{\mu\lambda})A^{\nu}+F^{\mu\lambda}\partial_{\lambda}(A^{\nu})[/tex]
[tex] -F^{\mu\sigma}\partial^{\nu}A_{\sigma}+\partial_{\lambda}(F^{\mu\lambda}A^{\nu})=-F^{\mu\sigma}\partial^{\nu}A_{\sigma}+\partial_{\sigma}(F^{\mu\sigma})A^{\nu}+F^{\mu\sigma}\partial_{\sigma}A^{\nu}[/tex]
[tex] -F^{\mu\sigma}\partial^{\nu}A_{\sigma}+\partial_{\lambda}(F^{\mu\lambda}A^{\nu})=F^{\mu\sigma}(-\partial^{\nu}A_{\sigma}+\partial_{\sigma}A^{\nu}) +\partial_{\sigma}(F^{\mu\sigma})A^{\nu}[/tex]
[tex] -F^{\mu\sigma}\partial^{\nu}A_{\sigma}+\partial_{\lambda}(F^{\mu\lambda}A^{\nu})=F^{\mu\sigma}F_{\sigma}^{\nu} +\partial_{\sigma}(F^{\mu\sigma})A^{\nu}[/tex]

This time nu seems to naturally come as an upper index. But what about my second term? It is not supposed to exist? I simply derived a product and I don't think this term vanishes because I remember it should define a current and generate Maxwell's equations from another problem I did.

I appreciate any comment and help.
 
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  • #2
For the first part you need to lower the indices as you stated and use the product rule.
 
  • #3
Hello, thank you for your answer, do you mean that this expression

[tex]\frac{\partial}{\partial(\partial_{\sigma}A_{\rho})} F^{\alpha\beta}[/tex]

is different from zero?

In that case how does that work when I perform a derivative with lower indices on an object with upper indices?
 
  • #4
Amentia said:
Hello, thank you for your answer, do you mean that this expression

[tex]\frac{\partial}{\partial(\partial_{\sigma}A_{\rho})} F^{\alpha\beta}[/tex]

is different from zero?

In that case how does that work when I perform a derivative with lower indices on an object with upper indices?

[tex] F^{\alpha \beta} = \eta^{\mu \alpha} \eta^{\nu \beta} F_{\mu \nu}[/tex]

[tex]\frac{\partial}{\partial(\partial_{\sigma}A_{\rho})} F^{\alpha\beta}= \eta^{\mu \alpha} \eta^{\nu \beta} \frac{\partial}{\partial(\partial_{\sigma}A_{\rho})} F_{\mu \nu}[/tex]
 
  • #5
Wow thank you for this equation, I believe it may solve all my factors 2 problem, and not only in this calculation but many other, when I calculate conjugate momenta from Lagrangians! Can you just remember me what eta is? I think I have seen somewhere that this is related to the metric tensor g but it is not defined in the book I am reading. I think they assume more knowledge of special relativity and tensor notations than I have.
 
  • #6
Sorry, should have read your post more carefully. Eta is what the flat spacetime metric is typically denoted by. Simply replace it with g and it's consistent with your notation. You can raise the index on the second part of your problem in the same way.
 
  • #7
So in the second problem, when I rise nu,
[tex]\delta_{\nu}^{\mu}[/tex]
is directly replaced by
[tex]g^{\mu\nu}[/tex]
?
 
  • #8
Correct.
 
  • #9
Do you know if there is a special reason why in the beginning the tensor is defined with low nu and then we rise it instead of having the tensor with all the indices up directly?
 
  • #10
Thank you anyway, I have to go to sleep, but I will take a look tomorrow to see if there are new answers.
 
  • #11
I'm not entirely sure. From what I recall, when we derive the energy-momentum tensor from the Lagrangian it's derived as a mixed tensor as in 1.41 here: http://www.damtp.cam.ac.uk/user/tong/qft/one.pdf. At the same time, I know a lot of identities regarding the tensor and equations using the tensor are given in terms of the energy-momentum tensor with both upper (or lower) indices. Perhaps that's why they're having you raise and lower it. Honestly, I'm just guessing and I don't think I have a satisfactory answer to this.
 

FAQ: Some trouble with relativistic notations

What is the concept of relativistic notations?

Relativistic notations are a mathematical framework used to describe the effects of relativity, specifically in the context of special relativity. They allow us to understand how time, space, and other physical quantities can vary depending on the relative speeds and frames of reference of observers.

Why is it important to use relativistic notations in scientific research?

Relativistic notations are crucial in scientific research because they accurately describe the behavior of physical systems at high speeds, where the effects of relativity become significant. Without these notations, our understanding of the universe would be incomplete and inaccurate.

What are some common challenges when working with relativistic notations?

One common challenge is the complexity of the equations involved, making them difficult to solve or manipulate. Another challenge is understanding and visualizing the concepts, as they often contradict our everyday experiences and intuitions.

How do relativistic notations differ from classical notations?

Relativistic notations take into account the principles of special relativity, such as the constancy of the speed of light and the relativity of simultaneity, while classical notations do not. Relativistic notations also involve the use of four-dimensional spacetime, whereas classical notations only use three dimensions of space.

What are some real-world applications of relativistic notations?

Relativistic notations are used in various fields, including particle physics, astrophysics, and engineering. They are essential in understanding the behavior of high-speed particles, such as those in particle accelerators, and in making precise calculations for satellite navigation systems.

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