12.07.2015 Views

Approaches to Quantum Gravity

Approaches to Quantum Gravity

Approaches to Quantum Gravity

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Questions and answers 153was that the question is spurious because an average Lorentz symmetry isalready manifested by the *individual* causet.Perhaps, however, you are implicitly asking whether quantum effects couldproduce a type of “averaging” that would remove the need for an intermediatenonlocality scale, or at least lower that scale down <strong>to</strong>ward the Planck length.That is an important question, but as far as I can see, we don’t yet have the<strong>to</strong>ols for answering it.• Q-D.Oriti-<strong>to</strong>R.Sorkin:1. I would like <strong>to</strong> draw your attention <strong>to</strong> the perspective offered on the issuesyou raise by Deformed Special Relativity models. On the one hand, it seems<strong>to</strong> me that they are a counterexample <strong>to</strong> your statement that the deformation ofthe dispersion relation for matter or gauge fields would necessarily imply theexistence of a state of absolute rest, i.e. a violation of Lorenz invariance. Nosuch state exists in DSR theories, which have a full 10-dimensional symmetrygroup in 4d, despite the deformation of dispersion relations that some of thesemodels predict.2. DSR models also seem good candidates for the effective dynamics of matterfields in discrete approaches <strong>to</strong> <strong>Quantum</strong> <strong>Gravity</strong> like spin foam modelsor group field theories. On the other hand, and exactly because they are fullyLorentz invariant in the above sense, DSR models, which are closely related<strong>to</strong> non-commutative geometry, seem <strong>to</strong> confirm your conclusion that “discretenessplus Lorentz invariance implies non-locality”. Indeed, as you say regardingnon-commutative geometry-based models, they seem <strong>to</strong> suggest that, at least insome cases, the modifications coming from <strong>Quantum</strong> <strong>Gravity</strong> <strong>to</strong> usual flat spacefield theories can be encoded in non-local field theory formulations. Also, theexistence of ∗ two ∗ scales of deformation of usual flat space physics, related <strong>to</strong>a minimal length scale and a maximal length scale (the cosmological constant),has been suggested as natural in the context of so called “doubly deformed (ortriply) special relativity”.3. It would be very interesting in this respect <strong>to</strong> obtain the dispersion relationfor some matter field propagating on a causal set and then compare this withthose studied in DSR models.4. Do you expect a phenomenon like UV/IR mixing in any field theory oncausal sets, according <strong>to</strong> the recent results on the D’Alembertian on a causal setthat you have described?5. How does the non-locality of causal sets compare, in your opinion, withthat suggested by Markopoulou, that identifies the discrepancy between macroscopic(i.e. metric-induced) locality and microscopic locality defined in termsof nearest-neighbor relations on the underlying graph (which is not, in itself, ageometric object)?

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