- #1
schieghoven
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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
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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