Crunching Away the Cosmological Constant Problem: Dynamical Selection of a Small $\Lambda$
Itay M. Bloch, Csaba Cs\'aki, Michael Geller, Tomer Volansky

TL;DR
This paper introduces a dynamical mechanism where regions with large cosmological constants rapidly crunch, leaving only small CC regions to survive, potentially explaining the small observed CC without requiring eternal inflation.
Contribution
It presents a concrete model based on a super-cooled phase transition that dynamically selects for small cosmological constants, offering a novel solution to the CC problem.
Findings
Large CC regions crunch quickly and do not survive.
Small CC regions are metastable and long-lived.
Predicts new relativistic degrees of freedom detectable in CMB experiments.
Abstract
We propose a novel explanation for the smallness of the observed cosmological constant (CC). Regions of space with a large CC are short lived and are dynamically driven to crunch soon after the end of inflation. Conversely, regions with a small CC are metastable and long lived and are the only ones to survive until late times. While the mechanism assumes many domains with different CC values, it does not result in eternal inflation nor does it require a long period of inflation to populate them. We present a concrete dynamical model, based on a super-cooled first order phase transition in a hidden conformal sector, that may successfully implement such a crunching mechanism. We find that the mechanism can only solve the CC problem up to the weak scale, above which new physics, such as supersymmetry, is needed to solve the CC problem all the way to the UV cutoff scale. The absence of…
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