Solving Electromagnetic Tensor & B-Field

StuartY
Messages
5
Reaction score
0
Hello, first off, I'm not sure if I put this question in the right place so sorry about that.
Given Bi = 1/2 εijk Fjk how would you find F in terms of B? I think you multiply through by another Levi-Civita, but then I don't know what to do after that. Any help would much appreciated.
 
Physics news on Phys.org
That's correct. When you multiple two levi-civitas, and end up with delta functions. Then you take advantage of F being antisymmetric.

B_i = \frac{1}{2} \epsilon_{ijk} F^{jk}
\epsilon^{imn} B_i = \frac{1}{2} \epsilon^{imn} \epsilon_{ijk} F^{jk}
\epsilon^{imn} B_i = \frac{1}{2} (\delta^m_j \delta^n_k - \delta^n_j \delta^m_k) F^{jk}
\epsilon^{imn} B_i = \frac{1}{2} (F^{mn} - F^{nm})
F^{nm} = - F^{mn}

after some relabeling:
\epsilon^{ijk} B_i = F^{jk}
 
Last edited:
DuckAmuck said:
That's correct. When you multiple two levi-civitas, you end up with a variety of results depending on how many indices are shared. In the case you want here, 2 are shared: \epsilon^{jkl} \epsilon_{ijk} = 2 \delta^{l}_i

B_i = \frac{1}{2} \epsilon_{ijk} F^{jk}
\epsilon^{jkl} B_i = \frac{1}{2} \epsilon^{jkl} \epsilon_{ijk} F^{jk}
\epsilon^{jkl} B_i = \frac{1}{2} 2 \delta^{l}_i F^{jk}
This is wrong, you can never have three of the same index when using the Einstein summation convention. You are using the same letter for some free indices as for some summation indices and then you confuse which is what. The thing to use is the standard epsilon-delta relation with only one index summed over and compute ##\epsilon_{mni} B_i##. I will leave the actual computation for the OP.
 
Orodruin said:
This is wrong, you can never have three of the same index when using the Einstein summation convention. You are using the same letter for some free indices as for some summation indices and then you confuse which is what. The thing to use is the standard epsilon-delta relation with only one index summed over and compute ##\epsilon_{mni} B_i##. I will leave the actual computation for the OP.

My bad. I guess I just remember the answer, and forgot how to do math. I fixed it.
 
Just use the identity
$$\epsilon_{ijk} \epsilon_{ilm}=\delta_{jl} \delta_{km} - \delta_{jm} \delta_{kl}.$$
The Hodge dual of a Hodge dual leads back to the original (up to signs), e.g.,
$$B_j=\epsilon_{jkl} F_{kl}=2(^{\dagger} F)_{j}$$
leads to
$$\epsilon_{abj}B_j=\epsilon_{jab} B_j=\epsilon_{jab} \epsilon_{jkl} F_{kl}=(\delta_{ak} \delta_{bl}-\delta_{al} \delta_{bk})) F_{kl}=F_{ab}-F_{ba}=2F_{ab}.$$
So indeed you have
$$^{\dagger \dagger} F=F.$$
Note that all this is in usual 3D Carrtesian notation. If you want to have this covariantly in Minkowski space you must be careful with the signs of the 4D Levi-Civita tensor. It also differs from one textbook to the other. So make sure you know the convention used in your textbook!
 
Thread 'Can this experiment break Lorentz symmetry?'
1. The Big Idea: According to Einstein’s relativity, all motion is relative. You can’t tell if you’re moving at a constant velocity without looking outside. But what if there is a universal “rest frame” (like the old idea of the “ether”)? This experiment tries to find out by looking for tiny, directional differences in how objects move inside a sealed box. 2. How It Works: The Two-Stage Process Imagine a perfectly isolated spacecraft (our lab) moving through space at some unknown speed V...
Does the speed of light change in a gravitational field depending on whether the direction of travel is parallel to the field, or perpendicular to the field? And is it the same in both directions at each orientation? This question could be answered experimentally to some degree of accuracy. Experiment design: Place two identical clocks A and B on the circumference of a wheel at opposite ends of the diameter of length L. The wheel is positioned upright, i.e., perpendicular to the ground...
According to the General Theory of Relativity, time does not pass on a black hole, which means that processes they don't work either. As the object becomes heavier, the speed of matter falling on it for an observer on Earth will first increase, and then slow down, due to the effect of time dilation. And then it will stop altogether. As a result, we will not get a black hole, since the critical mass will not be reached. Although the object will continue to attract matter, it will not be a...
Back
Top