Quantum field theory, gravity and cosmology in a fractal universe
Gianluca Calcagni

TL;DR
This paper introduces a fractal spacetime model for quantum field theory and gravity, achieving power-counting renormalizability with a Lorentz covariant action, and explores its implications for cosmology and the early universe.
Contribution
It presents a novel fractal spacetime framework for quantum fields and gravity, incorporating a Stieltjes measure and analyzing classical and quantum properties.
Findings
Spacetime flows from Hausdorff dimension 2 in the UV to D in the IR.
The scalar field exhibits a continuum of massive modes.
Ultraviolet cosmological solutions suggest early universe implications.
Abstract
We propose a model for a power-counting renormalizable field theory living in a fractal spacetime. The action is Lorentz covariant and equipped with a Stieltjes measure. The system flows, even in a classical sense, from an ultraviolet regime where spacetime has Hausdorff dimension 2 to an infrared limit coinciding with a standard -dimensional field theory. We discuss the properties of a scalar field model at classical and quantum level. Classically, the field lives on a fractal which exchanges energy-momentum with the bulk of integer topological dimension D. Although an observer experiences dissipation, the total energy-momentum is conserved. The field spectrum is a continuum of massive modes. The gravitational sector and Einstein equations are discussed in detail, also on cosmological backgrounds. We find ultraviolet cosmological solutions and comment on their implications for the…
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