Static, spherically symmetric Maxwell tensor

In summary, a static, spherically-symmetric Maxwell tensor has a vanishing magnetic field. The problem is that the solution requires the introduction of coordinate vectors on top of the Killing vectors already provided, which rules out magnetic monopoles.
  • #1
jdougherty
25
0

Homework Statement



Show that a static, spherically symmetric Maxwell tensor has a vanishing magnetic field.

Homework Equations



Consider a static, spherically-symmetric metric [itex]g_{ab}[/itex]. There are four Killing vector fields: a timelike [itex]\xi^{a}[/itex] satisfying
[tex]
\xi_{[a}\nabla_{b}\xi_{c]} = 0
[/tex]
and three vectors [itex](\ell_{i})^{a}[/itex] orthogonal to [itex]\xi^{a}[/itex] that generate rotations and commute with [itex]\xi^{a}[/itex]:
[tex]
[\xi, \ell_{i}]^{a} = 0, \qquad [\ell_{i}, \ell_{j}]^{a} = \epsilon^{ijk}(\ell_{k})^{a}
[/tex]
Given a two-form [itex]F_{ab}[/itex] that satisfies the source-free Maxwell's equations
[tex]
\nabla_{[a}F_{bc]} = 0, \qquad \nabla^{a}F_{ab} = 0,
[/tex]
Let [itex]\eta^{a} = (-\xi^{b}\xi_{b})^{-1/2}\xi^{a}[/itex], and define the electric and magnetic fields as
[tex]
E^{a} = {F^a}_{b}\eta^{b}, \qquad
B^{a} = \tfrac{1}{2}\epsilon^{abcd}\eta_{b}F_{cd}
[/tex]
where [itex]\epsilon_{abcd}[/itex] is a volume form, so
[tex]
F_{ab} = E_{[a}\eta_{b]} + \epsilon_{abcd}\eta^{c}B^{d}.
[/tex]
In order for [itex]F_{ab}[/itex] to share the symmetries of the spacetime, its Lie derivative along any of the Killing fields must vanish. Since it's closed, that means
[tex]
0 = \nabla_{[a}(F_{b]c}\lambda^{c}).
[/tex]
for [itex]\lambda^{a}[/itex] any of the Killing fields.

This ought to be enough information to show that [itex]B^{a} = 0[/itex], but I can't quite get there.

The Attempt at a Solution



Let [itex]\kappa = \xi^{a}\xi_{a}[/itex]. Expanding the Lie derivatives a bit, and using the fact that [itex]\xi^{a}[/itex] is hypersurface-orthogonal, you can show
[tex]
\xi^{c}\nabla_{[a}F_{b]c} = -\kappa^{-1}\xi^{c}F_{c[a}\nabla_{b]}\kappa + \kappa^{-1}F_{c[a}\xi_{b]}\nabla^{c}\kappa \\
(\ell_{i})^{c}\nabla_{[a}F_{b]c} = \tfrac{1}{2}F_{cb}\nabla_{a}(\ell_{i})^{c} - \tfrac{1}{2}F_{ca}\nabla_{b}(\ell_{i})^{c}
[/tex]
The RHS of that second one is begging to be contracted against some [itex](\ell_{j})^{a}(\ell_{k})^{b}[/itex] to make use of the commutation relations, but I can't find an appropriate selection of indices. I also tried taking the Lie derivative of [itex]F_{ab}[/itex] expressed in terms of [itex]E^{a}[/itex] and [itex]B^{a}[/itex], and the problem then comes down to calculating the commutator of the Killing vector and each of [itex]E^{a}[/itex] and [itex]B^{a}[/itex]. However, it wasn't particularly illuminating.

Thinking about it loosely, the spherical symmetry should be what forces [itex]B^{a} = 0[/itex], so you'd think that throwing [itex]B^{a}[/itex] and the second Lie derivative expression together and shaking sufficiently vigorously would do it. The problem I have there is that there's no obvious (to me) way to mix those two elements together.
 
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  • #2
I think you are making it much too complicated for yourself. Try to show/argue that in the coordinates adapted to ##\xi^{a}## and the spherical symmetry, the only non-zero independent component of an ##F_{ab}## which shares the aforementioned symmetries is ##F_{tr}## if we assume a vanishing magnetic monopole. Then since ##\xi^{\mu} = \delta^{\mu}_{t}##, ##B^{a}## must vanish identically in this coordinate representation (use the expression you wrote down for ##B^{a}## in terms of ##F_{ab}## and the 4-velocity of the observers measuring the EM field which in this case are the static observers) but if it vanishes identically in one coordinate system then it must vanish identically in all. Note that the key assumption here is the fact that ##F_{ab}## is static in a static space-time (so that there exists a family of observers which can remain "at rest" with respect to the static electromagnetic field and we know from regular EM that observers who are at rest with respect to a static EM field will see a pure E field).
 
  • #3
I am making it more complicated than it needs to be, but that's intentional. In coordinates the problem is relatively easy, but I'm interested in whether it can be done without introducing the coordinate vectors on top of the Killing vectors already provided.

I have another question about the magnetic monopole part. Doesn't a magnetic monopole mean that [itex]dF \not= 0[/itex], since it has to equal the magnetic current? Which means that magnetic monopoles are already ruled out. Wald also makes a point of this (Prob. 6.5), which confused me, since I could show that
[tex]
F_{ab} = 2A(r)\, (e_{0})_{[a}(e_{1})_{b]} + 2B(r)\, (e_{2})_{[a}(e_{3})_{b]}
[/tex]
only if [itex]B(r) = 0[/itex], but he also points out that [itex]B(r) \not= 0[/itex] means magnetic monopoles.
 

1. What is a static, spherically symmetric Maxwell tensor?

A static, spherically symmetric Maxwell tensor is a mathematical representation of the electric and magnetic fields in a vacuum surrounding a point charge that is stationary and evenly distributed in all directions. It is a tensor field that satisfies Maxwell's equations for electrostatics and magnetostatics in a spherical coordinate system.

2. How is a static, spherically symmetric Maxwell tensor calculated?

A static, spherically symmetric Maxwell tensor can be calculated by solving the differential equations that describe the electric and magnetic fields in a vacuum, subject to the boundary conditions of a stationary and spherically symmetric point charge. This involves using vector calculus and solving for the components of the tensor in a spherical coordinate system.

3. What is the significance of a static, spherically symmetric Maxwell tensor?

A static, spherically symmetric Maxwell tensor is significant because it represents a simplified and idealized version of the electric and magnetic fields around a point charge. It is often used as a theoretical model for understanding more complex systems, such as the behavior of charged particles in a plasma or the properties of electromagnetic waves.

4. What are some applications of a static, spherically symmetric Maxwell tensor?

A static, spherically symmetric Maxwell tensor has several applications in physics and engineering. It can be used to calculate the electric and magnetic fields in a vacuum surrounding a point charge, which is important for understanding the behavior of particles in particle accelerators. It is also used in the design and analysis of antennas, where the fields around a point charge are used to create and detect electromagnetic waves.

5. Are there any limitations to using a static, spherically symmetric Maxwell tensor?

Yes, there are limitations to using a static, spherically symmetric Maxwell tensor. It is a simplified model and does not account for the effects of time-varying electric and magnetic fields or the presence of other charged particles. It also assumes that the charge is evenly distributed in all directions, which may not always be the case. Therefore, it is important to use caution when applying this model to real-world situations and to consider more complex models when necessary.

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