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Axinos as Cold Dark Matter
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We show that axinos produced in the early Universe in the decay of the lightest neutralinos are a natural candidate for cold dark matter. We argue that axinos may well provide the main component of the missing mass in the Universe because their relic density is often comparable with the critical density.
Forward citations
Cited by 6 Pith papers
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Decaying Dark Matter Halo Abundance from a Revised Spherical Collapse Model
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BSFfast: Rapid computation of bound-state effects on annihilation in the early Universe
A public tool with new exact rescaling identities makes bound-state-formation cross sections with up to 100 excited states fast enough for routine dark-matter Boltzmann-solver scans.
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A frequentist view on the two-body decaying dark matter model
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Evading Dark Matter Bounds through NLSP-Assisted Freeze-Out with Long-Lived Signatures
In a U(1)B-L model with four chiral fermions, conversion-driven freeze-out lets a long-lived heavier fermion set the dark matter relic density while direct detection stays weak.
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A multi-axion model of inflation and dark matter
A 300-mode Kaluza-Klein axion tower is proposed as a unified inflaton and dark-matter sector, but the lightest state's quoted lifetime contradicts the paper's own decay-rate formula.
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Beyond the Veil: Charting WIMP Territories at the Neutrino Floor
Freeze-in, early matter domination, and fast-expanding cosmologies keep many WIMP models within reach of next-generation direct detection experiments at the neutrino floor.
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