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We discuss the formation mechanisms and structure of the superdense dark matter clumps (SDMC) and ultracompact minihaloes (UCMH), outlining the differences between these types of DM objects.
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V.I. Dokuchaev, Yu.N. Eroshenko, Stochastic Correlation Model of Galactic Bulge Velocity Dispersions and Central Black Holes Masses
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R.K. Sheth, H.J. Mo, G. Tormen, Ellipsoidal collapse and an improved model for the number and spatial distribution of dark matter haloes
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P. Ullio et al., Cosmological dark matter annihilations into γ \gamma -rays: A closer look
2002
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V.I. Dokuchaev, Yu.N. Eroshenko, Origin of Correlations between Central Black Holes Masses and Galactic Bulge Velocity Dispersions
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V. Berezinsky, V. Dokuchaev and Y. Eroshenko, Small-scale clumps in the galactic halo and dark matter annihilation
2003
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J. Diemand, B. Moore and J. Stadel, Earth-mass dark-matter haloes as the first structures in the early Universe
2005
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A.M. Green, S. Hofmann, D.J. Schwarz, The first WIMPy halos
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K.J. Mack, J.P. Ostriker and M. Ricotti, Growth of Structure Seeded by Primordial Black Holes
2007
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Y. Yang et al., The Abundance of New Kind of Dark Matter Structures
2011
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2011
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A.G. Doroshkevich, V.N. Lukash, E.V. Mikheeva, A solution of the problems of cusps and rotation curves in dark matter halos in the cosmological standard model
2012
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2013
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Y. Yang, G. Yang, and H. Zong, Dark Matter Decay and the Abundance of Ultracompact Minihalos
2013
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2013
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