Excellent discussion! All these solutions are also solutions for the free electromagnetic field, so that is the very end (once again) of the Higgs boson, assuming that an expensive figment of opiate nightmare has a beginning and end. The reason is that all these free field solutions have longitudinal components and are not U(1) gauge invariant. If the Higgs boson existed there would be no longitudinal solutions. These Beltrami solutions are observable in plasma flows, cosmology and hydrodynamics, they cause a river to meander. The simplest longitudinal solution is B(3), which is observed in the inverse Faraday effect as a static, longitudinal, magnetization. This was first observed fifty years ago at Havard in the group of the Nobel Laureate Bloembergen, who was co discoverer of the laser. The spectacular jet of a whirlpool galaxy is due to a B(3) type field, or a more complicated Beltrami longitudinal field.
Subj: Re: Animations and Particles
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Horst Eckardt hat am 26. Februar 2014 um 19:36 geschrieben:
Norman,
Obviously eqs. (18) and (21) are exactly the Bessel function example I have plotted and animated. Figs. 6 and 9 are density plots for the plane Z=0. I will provide such a plot. There are zero crossings as is explained in the text of the article. In Fig. 6 the zones have been levelled out in certain radius regions, in my plot they will look more continuous.
Horst
is there a formula describing a Birkeland current? Then we could check if it is obeys a Beltrami condition.
> Norman Page hat am 26. Februar 2014 um 17:13 geschrieben:
>
>
> Horst Another great animation. Check Fig 6 at
> http://electric-cosmos.org/BirkelandFields.pdf
> To see matter concentrations in Birkeland currents.
> Could be a X section through the electron shells of an atom. Like your
> animation.? Best Regards Norman Page