Cold dark matter heats up
Abstract
A principal discovery in modern cosmology is that standard model particles comprise only 5 per cent of the mass-energy budget of the Universe. In the ΛCDM paradigm, the remaining 95 per cent consists of dark energy (Λ) and cold dark matter. ΛCDM is being challenged by its apparent inability to explain the low-density `cores' of dark matter measured at the centre of galaxies, where centrally concentrated high-density `cusps' were predicted. But before drawing conclusions, it is necessary to include the effect of gas and stars, historically seen as passive components of galaxies. We now understand that these can inject heat energy into the cold dark matter through a coupling based on rapid gravitational potential fluctuations, explaining the observed low central densities.
- Publication:
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Nature
- Pub Date:
- February 2014
- DOI:
- 10.1038/nature12953
- arXiv:
- arXiv:1402.1764
- Bibcode:
- 2014Natur.506..171P
- Keywords:
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- Astrophysics - Cosmology and Extragalactic Astrophysics
- E-Print:
- Draft review as submitted to Nature on 1 Oct 2013. Accepted version scheduled for publication on 13 Feb 2014. In accordance with Nature policies, the accepted version cannot be posted until 13 Sep 2014