https://en.wikipedia.org/wiki/Renormalization_group
We are currently studying renormalization groups, in order to understand why gravity is non-renormalizable.
https://arxiv.org/abs/0709.3555
Assaf Shomer has written a 10 page explanation of the non-renormalizability of gravity.
Let us calculate a Feynman path integral, using some large number Λ as a cutoff for momenta.
In QED, the integral over a (vacuum polarization) loop diverges badly, but by setting a cutoff we can calculate results which are empirically correct! Why is that? What is going on?
Shomer requires that the partition function (= the generator for all correlation functions) stays the same regardless of the cutoff. The correlation functions tell us the physical behavior of the system. Why would a relatively arbitrary cutoff Λ give the correct behavior and not another slightly different cutoff Λ'?
Maybe the right model is to adjust the values of coupling constants for various cutoff sizes, in a way that the integral which yields the partition function has the same value regardless of the cutoff size?
Shomer derives in his paper the equation (13), which determines the RG flow, that is, the dependency we must set on the coupling constants on the cutoff Λ, in order to have the partition function integral the same regardless of the cutoff.
How does this compare to the intuitive idea of scaling self-similar systems, as outlined in the Wikipedia article?
In what way does a higher Λ mean analyzing the system in more precise detail? Like we would analyze the block spin example of Leo P. Kadanoff in the Wikipedia article?
The analogy between a higher cutoff and more detail is not clear. We have to think more about this.
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