Setting up a field theory (contra/covariant)

In summary, the conversation discusses the construction of the field strength tensor in the Reissner-Nordstrom solution to the Einstein field equations. The question arises about the use of contravariant and covariant indices in defining tensors, specifically the field strength tensor. It is noted that the metric can be used to raise and lower indices, but this may not always be the case for non-tensor objects. The use of Christoffel symbols, which are not tensors, is also mentioned.
  • #1
Pengwuino
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I'm trying to go through the Reissner-Nordstrom solution to the EFE's and since I'm trying to do this correctly, I find myself running into trouble about how to define everything.

I set my coordinates up as [tex]x^a = x^a(r,\theta,\phi,ct)[/tex]

Now, I need to use the fact that [tex]\nabla^b F_{ab} = 0[/tex] as I am looking for solutions in source-free space. However, the construction of the field strength tensor gets me. I'm attempting to follow Stephani's convention and he has his field strength tensor as

[tex]F^{ab} = \[
\left( {\begin{array}{*{20}c}
0 & {B_z } & { - B_y } & {E_x } \\
{ - B_z } & 0 & {B_x } & {E_y } \\
{B_y } & { - B_x } & 0 & {E_z } \\
{ - E_x } & { - E_y } & { - E_z } & 0 \\
\end{array}} \right)
\]
[/tex]

Now, the question I have is how would one know that this is how I should setup my field strength tensor? More to the point, why is it [tex]F^{ab}[/tex] and not [tex]F_{ab}[/tex]? My instinct tells me that you should simply define all of your tensors to start with either contravariantly or covariantly (ie. [tex]x^a, u^a, g^{ab}, F^{ab}, T^{ab}[/tex] etc.) and you work your geometry in with the covariant guys. Is this the right path to take?

Also, to what extent are you allowed to do things like [tex]A^{ab}B_{cabd} = A_{ab}B_c^{\;ab}_d[/tex]? It seems like in general you shouldn't be able to do that because, say in B, your a,b indices could be things in partial derivatives and your metric would have to act on them. On the other hand, I see things like [tex]F^{ab}F_{ab}[/tex] (the Maxwell field tensors) and know that it should equal [tex]F_{ab}F^{ab}[/tex]. Is it the fact that it's a scalar that makes them equal? Is it the anti-symmetry of [tex]F^{ab}[/tex]?
 
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  • #2
you can raise and lower indices using the metric so it doesn't really matter whether you define everything covariantly or contravariantly i.e.

with metric [tex] g_{ab} [/tex] and inverse metric [tex] g^{ab} [/tex]

[tex] F^{ab} = g^{ac} g^{bd} F_{cd} [/tex]

dummy indices you can lower and raise at your convenience in GR as long as they're in alternating positions
 
  • #3
Your a,b indices cannot be partial derivatives, since then the object in question wouldn't be a tensor under general coordinate transformations. They must be covariant derivatives, and since the covariant derivative of the metric is zero, you can raise and lower them with the metric without problems. Since [tex]F^{ab}[/tex] is antisymmetric in a and b, the Christoffel symbols actually cancel and the covariant derivatives reduce to partial, but that is a special case.
 
  • #4
What about something like the Christoffel symbols? They're constructed using partials. So I would think [tex]\Gamma_a^{\;b}_{\;c}A^a[/tex] is not necessarily the same as [tex]\Gamma^{ab}_{\;\;c}A_a[/tex].
 
  • #5
Christoffel symbols aren't tensors so you can't raise and lower their indices with the metric
 

FAQ: Setting up a field theory (contra/covariant)

What is a field theory?

A field theory is a mathematical framework used to describe physical phenomena in terms of fields, which are mathematical objects that represent physical quantities that vary in space and time. It is a fundamental concept in physics and is used to explain a wide range of phenomena, from electromagnetism to quantum mechanics.

What is the difference between contra and covariant in field theory?

In field theory, contra and covariant refer to the transformation of fields under changes in coordinates. Contra or contravariant fields transform in the opposite direction to the change in coordinates, while covariant fields transform in the same direction. This distinction is important in understanding the behavior of fields in different reference frames.

How do you set up a field theory?

The process of setting up a field theory involves several steps. First, you must identify the fields that will be used to describe the physical phenomena of interest. Next, you must determine the equations that govern the behavior of these fields, which are known as field equations. Finally, you must specify the boundary conditions and any other necessary constraints to solve the field equations and obtain solutions that correspond to physical reality.

What are some examples of field theories?

Some examples of field theories include classical field theories such as electromagnetism, general relativity, and quantum field theories such as the Standard Model. These theories are used to describe a wide range of physical phenomena, from the behavior of particles and forces at the quantum level to the curvature of spacetime due to massive objects.

How is field theory used in practical applications?

Field theory has many practical applications in physics, engineering, and other fields. For example, it is used in the development of technologies such as lasers, superconductors, and transistors. It is also used in the design and analysis of complex systems, such as fluid dynamics and materials science. In addition, field theory plays a crucial role in many areas of theoretical physics, from cosmology to particle physics.

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