Tuesday, September 2, 2014

Reconsider thie Mercury-Sun relativity problem

The problem, in Newton grammar, was something like this: In units, r became equal to three, and the integrals near the L1  went to unbound. Why? Because there is no natural process that knows pi. Nice work, Albert, for cracking the case and adding  2/3 multiplier appropriately, changing the rate of change in dx.

Why? Because Newton grammar is great, keep the symbols as long as possible then the integrals can be combined. Oh, you mean why did it happen at mercury?

G, it is almost a constant, its a number way down there, guaranteed above zero, but not quite a constant. As weak as G is, it still has a mediating unit sphere, the fuzzie, it has an L1 spot because its mediating unit circles hang out there. They can get congested, like any other sphere packer.

 Who is right? Did my grid spheres become congested, or did Albert's integral hit zero? If space stretches, uniformly, then little bubbles can group in bunches. I am not saying L1 fuzzies cause gravity, I say they just keep phase.

Like when one of these stars explodes. The L1 get congested, they have 6e6 meter wavelength along their only degree of freedom. The fuzzies keep time, and when congested do the swirl, jump the p/q bounds. Gravity, just as weak as ever, just goes along with the fuzzies. A discrete but just as correct. If you want integrals, just derive them from the short order difference equations.

What is the fuzzy lifetime? I bet they streak through the L spots and live a short life and return to lower density vacuum.  The L spot is how the fuzzies maintain the gravity radial alignment.






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