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arXiv · astro-ph/0106251

Cold Dark Matter Halos Must Burn

P. Salucci·A. Borriello
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Abstract

High-quality optical rotation curves for a sample of low-luminosity spirals evidence that the dark halos around galaxies are inconsistent with the output of proper CDM simulations. In fact, dark halos enveloping stellar disks are structures with approximately a constant density out to the optical edges. This is in strong disagreement with the characteristic rho(r) ~ r^(-1.5) CDM regime and severely challenges the "standard" CDM theory, also because the halo density appears to be heated up, at gross variance with the hierarchical evolution of collision-free particles.

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P. Salucci, A. Borriello. 2001-10-29. Cold Dark Matter Halos Must Burn. https://doi.org/10.1007/10856495_82

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