Super heavy dark matter from inflationary Schwinger production
Mar Bastero-Gil, Paulo B. Ferraz, Lorenzo Ubaldi, Roberto Vega-Morales

TL;DR
This paper proposes a mechanism where dark electrons are produced during inflation via the Schwinger effect in a dark U(1) gauge field, potentially explaining dark matter with masses from 100 GeV to 10^{17} GeV, independent of thermal processes.
Contribution
It introduces a novel inflationary Schwinger production mechanism for super heavy dark matter, distinct from gravitational production, with detailed analysis of non-thermal, decoupled dark sector evolution.
Findings
Dark electrons can account for dark matter abundance over a wide mass range.
Production is efficient even for masses exceeding the Hubble scale at inflation's end.
Dark sector remains decoupled from Standard Model, with relic abundance set by initial inflationary conditions.
Abstract
We consider a simple setup with a dark sector containing dark electrons charged under an abelian gauge symmetry. We show that if the massless dark photon associated to the is produced during inflation in such a way as to form a classical dark electric field, then dark electron-positron pairs are also produced close to the end of inflation via the Schwinger effect even if they are very massive. For large enough dark electric force, dark electrons with masses larger than the Hubble scale can be produced which are non-relativistic at production and throughout their cosmic evolution. They can account for the dark matter abundance today for masses in the range 100 GeV to GeV and up to six orders of magnitude larger than the Hubble scale at the end of inflation where purely gravitational production is exponentially suppressed. We examine the regime where the…
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Taxonomy
TopicsCosmology and Gravitation Theories · Dark Matter and Cosmic Phenomena · Geophysics and Gravity Measurements
