Special Relativity: A^μ_ν Differences Explained

In summary, there are three expressions that can denote components of a 2nd-rank tensor: A^{\mu}_{\hspace{0.2cm} \nu}, A^{\hspace{0.2cm} \mu}_{\nu}, and A^{\mu}_{\nu}. The first two are correct and can be used interchangeably, while the last one should be avoided due to the lack of indication for horizontal placement of indices. Tensors are not matrices and matrices are not tensors, but tensors can be represented by matrices in some basis. When representing a tensor as a matrix, the first index is typically the row and the second is the column. However, it is important to be cautious when contracting indices
  • #1
LagrangeEuler
717
20
Can someone explain me difference between
[tex]A^{\mu}_{\hspace{0.2cm} \nu}[/tex]
[tex]A^{\hspace{0.2cm} \mu}_{\nu}[/tex]
and
[tex]A^{\mu}_{\nu}[/tex]?
 
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  • #2
The first two expressions are correct and usually denote components of a 2nd-rank tensor. You can lower and raise indices with the metric components ##g_{\mu \nu}## and ##g^{\mu \nu}##, respectively, i.e., you have
$${A_{\nu}}^{\mu} = g_{\nu \sigma} g^{\mu \rho} {A^\sigma}_{\rho}.$$
The last expression should be avoided, because the horizontal placement of the indices is not indicated. It's ok if the tensor ##A## is symmetric, i.e., if ##A_{\mu \nu}=A_{\nu \mu}##, because (only!) then
$${A^{\mu}}_{\nu} = g^{\mu \rho} A_{\rho \nu} = g^{\mu \rho} A_{\nu \rho} ={A_{\nu}}^{\mu},$$
and the horizontal ordering is not important.
 
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  • #4
vanhees71 said:
The first two expressions are correct and usually denote components of a 2nd-rank tensor. You can lower and raise indices with the metric components ##g_{\mu \nu}## and ##g^{\mu \nu}##, respectively, i.e., you have
$${A_{\nu}}^{\mu} = g_{\nu \sigma} g^{\mu \rho} {A^\sigma}_{\rho}.$$
The last expression should be avoided, because the horizontal placement of the indices is not indicated. It's ok if the tensor ##A## is symmetric, i.e., if ##A_{\mu \nu}=A_{\nu \mu}##, because (only!) then
$${A^{\mu}}_{\nu} = g^{\mu \rho} A_{\rho \nu} = g^{\mu \rho} A_{\nu \rho} ={A_{\nu}}^{\mu},$$
and the horizontal ordering is not important.
Is there some connection with matrices? For instance, if we have two indices.
[tex]A^{\mu}_{\hspace{0.2cm}\nu}[/tex] what is the row and what is the column? And in this case
[tex]A^{\hspace{0.2cm}\mu}_{\nu}[/tex] what is the row and what is the column?
 
  • #5
Tensors are not matrices and matrices are not tensors. Tensors (of rank 2) may be represented by matrices in some basis but it is then up to you to define how indices correspond to rows and columns in a consistent manner.
 
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  • #6
LagrangeEuler said:
And in this case [tex]A^{\hspace{0.2cm}\mu}_{\nu}[/tex] what is the row and what is the column?
Typically when in a given basis you represent a tensor as a matrix the first index (on the left) is the row and the second the column. So in your example ##\nu## is the row and ##\mu## the column.
 
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  • #7
I'd repeat Orodruin's caution. Any rank 2 tensor can be represented as a matrix (4×4 in relativity), and it's quite common to get metric tensors represented like this. But there isn't a way to notate upper and lower indices in that form, so it isn't clear what can be legally contracted with what and it's easy to end up writing a matrix equation that contracts over two lower indices. That's difficult to debug, so you do it at your own risk.
 
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FAQ: Special Relativity: A^μ_ν Differences Explained

What is special relativity?

Special relativity is a theory developed by Albert Einstein in 1905 that describes the relationship between space and time in the absence of gravity. It explains how the laws of physics are the same for all observers in uniform motion, and how the speed of light is constant for all observers.

What does A^μ_ν represent in special relativity?

In special relativity, A^μ_ν is a tensor that represents the electromagnetic field. It is used to describe the electric and magnetic fields in a unified way, and is an essential component in understanding the theory of relativity.

What are the differences between A^μ_ν in special relativity and A^μ_ν in general relativity?

The main difference between A^μ_ν in special relativity and general relativity is that in special relativity, A^μ_ν represents the electromagnetic field, while in general relativity it represents the gravitational field. In general relativity, A^μ_ν is also a symmetric tensor, while in special relativity it is not necessarily symmetric.

How does special relativity explain time dilation and length contraction?

Special relativity explains time dilation and length contraction as consequences of the relativity of simultaneity and the constancy of the speed of light. Time dilation occurs when an observer in motion experiences time passing slower than an observer at rest, while length contraction occurs when an object in motion appears shorter in the direction of motion to an observer at rest.

How has special relativity been confirmed by experiments?

Special relativity has been confirmed by numerous experiments, including the famous Michelson-Morley experiment, which showed that the speed of light is constant in all directions. Other experiments, such as the Hafele-Keating experiment and the GPS system, have also confirmed the predictions of special relativity. Its accuracy has been verified to a high degree, making it one of the most well-supported theories in physics.

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