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Old Jun26-09, 12:07 PM                  #1
schieghoven

schieghoven is Offline:
Posts: 53
Electromagnetic version of the positive energy theorem?

Hello,

I've been quite avidly reading about one of the spectacular recent joint achievements of physics and pure math. The positive energy theorem [1,2,3] concerns the large-distance asymptotic behaviour of the gravitational field due to a localised distribution of mass-energy. I think I paraphrase the theorem correctly to say that, provided the source is physical (energy density T_00 is everywhere positive in every local Lorentz frame), then the energy of the system, as inferred from the large-distance gravitational field, is also positive. A neat and powerful result.

I was wondering if a similar result holds for electromagnetic theory. If we take Maxwell's equations and again impose that the source is physical (the current J_\mu is future-timelike), does this place some analogous constraint on the large-distance behaviour of the associated electromagnetic field? This linear system should presumably be much easier than the hard-core nonlinearity of Einstein GR, but nothing obvious jumped out at me.

Thanks,

Dave

* [1] Schoen, R. and Yau, S-T., Commun. Math. Phys, 65 (1979) 45
* [2] Witten, E., Commun. Math. Phys. 80 (1981) 381
* [3] Kazdan, J., Seminaire N. Bourbaki, 24 (1982) 315, Exp 593

[3], a review article, is publicly available at http://www.numdam.org/numdam-bin/browse?j=SB
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Old Jun26-09, 04:46 PM                  #2
Stingray

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Posts: 625
Re: Electromagnetic version of the positive energy theorem?

Assuming that the current density is nonzero and future-directed timelike implies that the system's charge (measured either normally or via the asymptotic fields) is non-negative. This is pretty easy to see from the first method:

LaTeX Code: <BR>q = \\int_\\Sigma J^a \\mathrm{d}S_a > 0.<BR>

Using Stoke's theorem together with Maxwell's equations shows that this also appears in the field at infinity:

LaTeX Code: <BR>q = \\frac{1}{8\\pi} \\int_{\\partial \\Sigma} F^{ab} \\mathrm{d}S_{ab} .<BR>

Unlike in the gravitational case, this kind of restriction on the source is not consistent with observations. Spacelike currents are actually very common. Think of an ordinary wire. There's no net charge, yet there is a 3-current. The 4-current is therefore spacelike. This is possible because there are both positive and negative charges.
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