Multi-component Dark Matter and small scale structure formation

Abstract We consider the evolution of non-thermal dark matter perturbations in models which contain both Weakly Interacting Massive Particles (WIMPs) and axions. Using constraints from existing observations we examine the percentage of WIMPs and axions that may comprise the cosmological dark matter...

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Bibliographic Details
Main Authors: Robert Wiley Deal, Kishan Sankharva, Kuver Sinha, Scott Watson
Format: Article
Language:English
Published: SpringerOpen 2024-02-01
Series:Journal of High Energy Physics
Subjects:
Online Access:https://doi.org/10.1007/JHEP02(2024)085