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arXiv · 2605.16587

3d QFT IR divergences as UV divergences in 4d Holographic Cosmology

Matheus Cravo·Horatiu Nastase
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Abstract

In this paper we consider IR divergences in a 3d toy model field theory for 4d holographic cosmology, and we analyze them by introducing a mass term in a way that preserves a certain form of the generalized conformal structure. This allows us to compute 2- and 3-point functions at 2-loops and study their IR structure below the mass scale, from which we argue for a possible IR finiteness beyond perturbation theory, consistent with lattice results. In the holographically dual 4d cosmology, this corresponds to UV finiteness, i.e., the absence of cosmological singularities. The 3d IR field theory methods could be extended beyond this specific application.

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Matheus Cravo, Horatiu Nastase. 2026-05-15. 3d QFT IR divergences as UV divergences in 4d Holographic Cosmology. https://arxiv.org/abs/2605.16587

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