Inflaton Clusters and Inflaton Stars

Abstract

In a broad class of scenarios, inflation is followed by an extended era of matter-dominated expansion during which the inflaton condensate is nonrelativistic on subhorizon scales. During this phase density perturbations grow to the point of nonlinearity and collapse into bound structures. This epoch strongly resembles structure formation with ultra-light axion-like particles. This parallel permits us to adapt results from studies of cosmological structure formation to describe the nonlinear dynamics of this post-inflationary epoch. We show that the inflaton condensate fragments into "inflaton clusters", analogues of axion dark matter halos in present-day cosmology. Moreover, solitonic objects or "inflaton stars" can form inside these clusters, leading to density contrasts as large as $10^6$ in the post-inflationary universe.

11 pages; 3 figures; reformatted, references added, minor changes

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• Multifield Ultralight Dark Matter
• Schrödinger-Poisson Solitons: Perturbation Theory
• Soliton Formation and the Core-Halo Mass Relation: An Eigenstate Perspective
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• Soliton boson stars, Q-balls and the causal Buchdahl bound