Banks-Zaks Cosmology, Inflation, and the Big Bang Singularity
Michal Artymowski, Ido Ben-Dayan, Utkarsh Kumar

TL;DR
This paper explores how Banks-Zaks theory influences cosmological evolution, proposing non-singular bouncing and cyclic universes that challenge traditional Big Bang models by violating classical energy conditions.
Contribution
It introduces a novel non-singular cosmological model based on Banks-Zaks theory's anomalous dimension, avoiding the Big Bang singularity without scalar fields.
Findings
Banks-Zaks theory leads to non-singular bouncing universes.
The model includes inflation without a Big Bang singularity.
Violates the Null Energy Condition near bounces.
Abstract
We consider the thermodynamical behavior of Banks-Zaks theory close to the conformal point in a cosmological setting. Due to the anomalous dimension, the resulting pressure and energy density deviate from that of radiation and result in various interesting cosmological scenarios. Specifically, for a given range of parameters one avoids the cosmological singularity. We provide a full "phase diagram" of possible Universe evolution for the given parameters. For a certain range of parameters, the thermal averaged Banks-Zaks theory alone results in an exponentially contracting universe followed by a non-singular bounce and an exponentially expanding universe, i.e. \textit{Inflation without a Big Bang singularity}, or shortly termed "dS Bounce". The temperature of such a universe is bounded from above and below. The result is a theory violating the classical Null Energy Condition (NEC).…
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