Saxion Cosmology for Thermalized Gravitino Dark Matter
arXiv:1703.09796 · doi:10.1007/JHEP07(2017)125
Abstract
In all supersymmetric theories, gravitinos, with mass suppressed by the Planck scale, are an obvious candidate for dark matter; but if gravitinos ever reached thermal equilibrium, such dark matter is apparently either too abundant or too hot, and is excluded. However, in theories with an axion, a saxion condensate is generated during an early era of cosmological history and its late decay dilutes dark matter. We show that such dilution allows previously thermalized gravitinos to account for the observed dark matter over very wide ranges of gravitino mass, keV < < TeV, axion decay constant, GeV < < GeV, and saxion mass, 10 MeV < < 100 TeV. Constraints on this parameter space are studied from BBN, supersymmetry breaking, gravitino and axino production from freeze-in and saxion decay, and from axion production from both misalignment and parametric resonance mechanisms. Large allowed regions of remain, but differ for DFSZ and KSVZ theories. Superpartner production at colliders may lead to events with displaced vertices and kinks, and may contain saxions decaying to or a pair of Standard Model fermions. Freeze-in may lead to a sub-dominant warm component of gravitino dark matter, and saxion decay to axions may lead to dark radiation.
30 pages, 4 figures
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- Displaced new physics at colliders and the early universe before its first second
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- Axion Dark Radiation: Hubble Tension and Hyper-kamiokande Neutrino Experiment
- The Supersymmetric R-Parity Violating Dine-Fischler-Srednicki-Zhitnitsky Axion Model
- Searching for Metastable Particles with Sub-Millimeter Displaced Vertices at Hadron Colliders
- Common Origin of Warm Dark Matter and Dark Radiation
- A QCD R-Axion
- Fingerprints of freeze-in dark matter in an early matter-dominated era