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The evaporation of primordial black holes (PBH) with masses ranging from $\sim 10^{-1}$ to $\sim 10^9$ g could have generated the whole observed dark matter (DM) relic density.
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M. Khlopov, A. Barrau and J. Grain, Gravitino production by primordial black hole evaporation and constraints on the inhomogeneity of the early universe , Class. Quant. Grav. 23
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F. De Bernardis, L. Pagano and A. Melchiorri, New constraints on the reheating temperature of the universe after WMAP-5 , Astropart. Phys. 30
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M. Farina, D. Pappadopulo, J.T. Ruderman and G. Trevisan, Phases of Cannibal Dark Matter , JHEP 12
2016
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N. Bernal and X. Chu, ℤ 2 \mathbb{Z}_{2} SIMP Dark Matter , JCAP 01
2016
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S.-M. Choi, H.M. Lee and M.-S. Seo, Cosmic abundances of SIMP dark matter , JHEP 04
2017
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X. Chu and C. Garcia-Cely, Self-interacting Spin-2 Dark Matter , Phys. Rev. D 96
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M. Heikinheimo, T. Tenkanen and K. Tuominen, WIMP miracle of the second kind , Phys. Rev. D 96
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H. Deng and A. Vilenkin, Primordial black hole formation by vacuum bubbles , JCAP 12
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Particle Data Group
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