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Meaning of "low energy" in loop quantum gravity
In the recent Immirzi parameter thread we accumulated some evidence that to resolve and/or clarify the issues raised there, it would be necessary to have an understanding of the flow to low energy or the flow from micro to macro in loopy models of gravity. This statement is almost trivial in field theory since we know very well now that low energy parameters and degrees of freedom need not be anything like those at high energy. However, it seems quite non-trivial in the context of loopy gravity.
What I have in mind is the question: what "energy" are we flowing to low values of in loopy gravity models? Perhaps energy is the wrong word in general, but it must eventually become the right word in some limits e.g. semiclassical gravity with weak quantum corrections around flat space. So I would like to discuss this issue, namely, what do we do know about generalized renormalization in loopy gravity models? How to define it, the difference between micro and macro, connection to semiclassical limit, universality, etc.
Also, I would just like to note that this problem is less severe or even absent for some models of emergent spacetime. Fotini's quantum graphity is one example where time is not emergent, energy is a sensible quantity, and we can meaningfully speak of the flow to low energy, although not perhaps the flow to long wavelengths in an unambiguous way.
It might also be interesting to discuss renormalization in other models of quantum gravity, for example, perturbative string theory or holographic duality. Indeed, within holographic duality, we have a good understanding of what renormalization in the dual field theory corresponds to in the bulk, but how should we think about renormalization in the bulk (or should we)?
In the recent Immirzi parameter thread we accumulated some evidence that to resolve and/or clarify the issues raised there, it would be necessary to have an understanding of the flow to low energy or the flow from micro to macro in loopy models of gravity. This statement is almost trivial in field theory since we know very well now that low energy parameters and degrees of freedom need not be anything like those at high energy. However, it seems quite non-trivial in the context of loopy gravity.
What I have in mind is the question: what "energy" are we flowing to low values of in loopy gravity models? Perhaps energy is the wrong word in general, but it must eventually become the right word in some limits e.g. semiclassical gravity with weak quantum corrections around flat space. So I would like to discuss this issue, namely, what do we do know about generalized renormalization in loopy gravity models? How to define it, the difference between micro and macro, connection to semiclassical limit, universality, etc.
Also, I would just like to note that this problem is less severe or even absent for some models of emergent spacetime. Fotini's quantum graphity is one example where time is not emergent, energy is a sensible quantity, and we can meaningfully speak of the flow to low energy, although not perhaps the flow to long wavelengths in an unambiguous way.
It might also be interesting to discuss renormalization in other models of quantum gravity, for example, perturbative string theory or holographic duality. Indeed, within holographic duality, we have a good understanding of what renormalization in the dual field theory corresponds to in the bulk, but how should we think about renormalization in the bulk (or should we)?