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arXiv · 1904.07876

Cosmological constant: relaxation vs multiverse

Alessandro Strumia·Daniele Teresi
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Abstract

We consider a scalar field with a bottom-less potential, such as $g^3 ϕ$, finding that cosmologies unavoidably end up with a crunch, late enough to be compatible with observations if $g \lesssim 1.2 H_0^{2/3} M_{\rm Pl}^{1/3}$. If rebounces avoid singularities, the multiverse acquires new features; in particular probabilities avoid some of the usual ambiguities. If rebounces change the vacuum energy by a small enough amount, this dynamics selects a small vacuum energy and becomes the most likely source of universes with anthropically small cosmological constant. Its probability distribution could avoid the gap by 2 orders of magnitude that seems left by standard anthropic selection.

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Alessandro Strumia, Daniele Teresi. 2019-08-29. Cosmological constant: relaxation vs multiverse. https://doi.org/10.1016/j.physletb.2019.134901

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