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That's what I said in my first post.Haelfix said:1) Background independance here means a weak form found eg in semiclassical gravity or in perturbative string theory. Namely that after you perform a background field split, the metric g is left arbitrary and not fixed. In other words you can carry it through to the end of the calculation, and don't need to make many assumptions about the nature of the geometry a priori. Whereas in previous numerical work, certain boundary conditions and symmetries needed to be there (by hand) in order to make the calculation tractable (eg spherically symmetric spacetimes or perhaps flat space) and you have to start from scratch if you wanted something a little different.
I thought it was just another perturbative algorithm. I didn't look into the paper, but since you talk about heat kernel, I assumed everything they do is euclidean gravity right ?Haelfix said:So while this is a technical advantage (indeed it is one of the virtues of the heat kernel expansions pionered by De Witt) it is still merely another algorithm and expansion/truncation method and merely reverifies the fixed point structure found in previous papers using the functional exact renormalization group methods.
Right, you have no control over the physics.Haelfix said:The fundamental problem with this whole business, and what basically most of the theorists I have asked state, boils down to universality classes. In other words, the theory you started with, is not necessarily what you end up with. Whenever you do violence to the perturbation expansion in step 3, you have to really worry about whether or not step 4 is probing something *else* (possibly spurious fixed points for instance) outside of what you are interested in.
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