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Similar

C. Cheung, G. Elor, L. J. Hall, and P. Kumar, Origins of Hidden Sector Dark Matter II: Collider Physics
Original
2011
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N. D. Christensen, P. de Aquino, C. Degrande, C. Duhr, B. Fuks, et al., A Comprehensive approach to new physics simulations
Original
2011
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L. Bergström, Dark matter evidence, particle physics candidates and detection methods
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2012
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Then

M. S. Madhavacheril, N. Sehgal, and T. R. Slatyer, Current Dark Matter Annihilation Constraints from CMB and Low-Redshift Data
Original
2014
Later among the works it cites.
M. Blennow, E. Fernandez-Martínez, and B. Zaldivar, Freeze-in through portals
Original
2014
Later among the works it cites.
E. Bulbul, M. Markevitch, A. Foster, R. K. Smith, M. Loewenstein, et al., Detection of An Unidentified Emission Line in the Stacked X-ray spectrum of Galaxy Clusters
Original
2014
Later among the works it cites.
A. Boyarsky, O. Ruchayskiy, D. Iakubovskyi, and J. Franse, Unidentified Line in X-Ray Spectra of the Andromeda Galaxy and Perseus Galaxy Cluster
Original
2014
Later among the works it cites.
P. Bechtle, S. Heinemeyer, O. Stål, T. Stefaniak, and G. Weiglein, Probing the Standard Model with Higgs signal rates from the Tevatron, the LHC and a future ILC

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2015

Production Regimes for Self-Interacting Dark Matter

Bernal, Nicolas, Chu, Xiaoyong, Garcia-Cely, Camilo et al.

Understand

In the context of Self-Interacting Dark Matter as a solution for the small-scale structure problems, we consider the possibility that Dark Matter could have been produced without being in thermal equilibrium with the Standard Model bath.

We discuss one by one the following various dark matter production regimes of this kind: freeze-in, reannihilation and dark freeze-out.
We exemplify how these mechanisms work in the context of the particularly simple Hidden Vector Dark Matter model.
In contrast to scenarios where there is thermal equilibrium with the Standard Model bath, we find two regimes which can easily satisfy all the laboratory and cosmological constraints.