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atyy said:I had in mind the landscape of theories in any theory of pure gravity that can couple arbitrarily to matter. This is the "bewildering number of possibilities" Percacci mentions in http://arxiv.org/abs/0911.0386
"Let us assume for a moment that this ambitious goal can be achieved, and that pure gravity can be shown to be asymptotically safe. Still, from the point of view of phenomenology, we could not be satisfied because the real world contains also dozens of matter fields ... More generally the asymptotic safety program requires that the fully interacting theory of gravity and matter has a FP with the right properties. Given the bewildering number of possibilities, in the search for such a theory one needs some guiding principle."
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But Atyy, you have not offered any evidence of a landscape problem! Your paper shows Percacci immediately applying a readily available selection principle to narrow down the (comparatively modest) range of possibilities.
He may have used the word "bewildering" at the start of the paper to highlight the challenge he is undertaking, but he does not act in any way bewildered. Nor does he desperately invoke "anthropics" as Susskind did for string in 2003. He forges right ahead and applies the Wetterich method of "effective average action" ---see the blue highlight in the quote below.
At least wait until the AsymSafe people cry "Help!" before you conclude they are in trouble.
Many seem prone to an unfortunate tendency, whenever one hears of some snag or drawback in the string program, to project it on all the other approaches and believe (or pretend) they have it worse. Either it's not a problem, or string doesn't really have the problem, or all the other approaches have it worse.
You have probably picked up on this. I recall a couple of years back a discussion of the "no background geometry" feature where I was told seriously that LQG was not background independent and that string was much more independent than everybody else (LQG, CDT).
There is a kind of compulsion to bend the words so that it always comes out like that.
Here's the context of the Percacci passage quoted above, in case anyone is interested:
==quote Percacci 0911. ==
The original motivation for this work comes fromthe progress that has been made in recent years towards understanding the UVbehaviour of gravity. It seems that pure gravity possesses a Fixed Point (FP) with the right properties to make it asymptotically safe, or in other words nonperturbatively renormalizable [2, 3, 4, 5, 6, 7, 8, 9, 10, 11, 12, 13, 14, 15, 16, 17, 18, 19, 39] (see also [20] for reviews). Let us assume for a moment that this ambitious goal can be achieved, and that pure gravity can be shown to be asymptotically safe. Still, from the point of view of phenomenology, we could not be satisfied because the real world contains also dozens of matter fields that interact in other ways than gravitationally, and their presence affects also the quantum properties of the gravitational field, as is known since long[21].
Indeed, in a first investigation along these lines, it was shown in [22] that the presence of minimally coupled (i.e. nonself-interacting) matter fields shifts the position of the gravitational FP and the corresponding critical exponents. In some cases the FP ceases to exist, so it was suggested that this could be used to put bounds on the number of matter fields of each spin.
More generally the asymptotic safety program requires that the fully interacting theory of gravity and matter has a FP with the right properties. Given the bewildering number of possibilities, in the search for such a theory one needs some guiding principle. One possibility that naturally suggests itself is that all matter self-interactions are asymptotically free[33]. Then, asymptotic safety requires the existence of a FP where the matter couplings approach zero in the UV, while the gravitational sector remains interacting.
We will call such a FP a “Gaussian Matter FP” or GMFP. Following a time honored tradition,as a first step in this direction, scalar self interactions have been studied in [34, 35]. Here we pursue that study further. The tool that we use is the Wetterich equation, an exact renormalization group (RG) flow equation for a type of Wilsonian effective action Γk , called the “effective average action”. This functional, depending on an external energy scale k, can be formally defined by...
==endquote==
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