The Core‐Cusp Problem
2009; Hindawi Publishing Corporation; Volume: 2010; Issue: 1 Linguagem: Inglês
10.1155/2010/789293
ISSN1687-7977
Autores Tópico(s)Dark Matter and Cosmic Phenomena
ResumoThis paper gives an overview of the attempts to determine the distribution of dark matter in low surface brightness disk and gas-rich dwarf galaxies, both through observations and computer simulations. Observations seem to indicate an approximately constant dark matter density in the inner parts of galaxies, while cosmological computer simulations indicate a steep power-law-like behaviour. This difference has become known as the "core/cusp problem", and remains one of the unsolved problems in small-scale cosmology.
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