Special Relativity: A^μ_ν Differences Explained

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LagrangeEuler
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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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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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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?
 
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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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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