Quantum spectral dimension in quantum field theory
arXiv:1408.0199 · doi:10.1142/S0218271816500589
Abstract
We reinterpret the spectral dimension of spacetimes as the scaling of an effective self-energy transition amplitude in quantum field theory (QFT), when the system is probed at a given resolution. This picture has four main advantages: (a) it dispenses with the usual interpretation (unsatisfactory in covariant approaches) where, instead of a transition amplitude, one has a probability density solving a nonrelativistic diffusion equation in an abstract diffusion time; (b) it solves the problem of negative probabilities known for higher-order and nonlocal dispersion relations in classical and quantum gravity; (c) it clarifies the concept of quantum spectral dimension as opposed to the classical one. We then consider a class of logarithmic dispersion relations associated with quantum particles and show that the spectral dimension of spacetime as felt by these quantum probes can deviate from its classical value, equal to the topological dimension . In particular, in the presence of higher momentum powers it changes with the scale, dropping from in the infrared (IR) to a value in the ultraviolet (UV). We apply this general result to Stelle theory of renormalizable gravity, which attains the universal value for any dimension .
26 pages, 3 figures; v2: discussion clarified and improved at several points, typos corrected, results unchanged; v3: some material confined to an appendix, discussion streamlined, results unchanged
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- Spontaneous Dimensional Reduction in Quantum Gravity
- On the UV dimensions of Loop Quantum Gravity
- Deformed symmetries in noncommutative and multifractional spacetimes
- Standard Model in multiscale theories and observational constraints
- Dimensional reduction in manifold-like causal sets
- Dimensional flow in the kappa-deformed space-time
- Ultraviolet dimensional reduction of spacetime with zero-point length