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Self-interacting dark matter : ウィキペディア英語版 | Self-interacting dark matter In astrophysics self-interacting dark matter is a hypothetical form of dark matter consisting of particles with strong self-interactions. This type of dark matter was postulated to resolve a number of conflicts between observations and simulations on the galactic scale and smaller.〔D. N. Spergel and P. J. Steinhardt, ''Observational evidence for self-interacting cold dark matter'', Phys. Rev. Lett. 84, 3760-3763 (2000) (preprint ).〕 〔B. D. Wandelt, R. Dave, G. R. Farrar, P. C. McGuire, D. N. Spergel and P. J. Steinhardt, ''Self-Interacting Dark Matter'', Marina del Rey 2000, Sources and detection of dark matter and dark energy in the universe, 263 (2000), (preprint ).〕 Self-interacting dark matter has also been postulated as an explanation for the DAMA annual modulation signal.〔S. Mitra, ''Has DAMA detected self-interacting dark matter?'', Phys. Rev. D 71, 121302 (2005) (preprint ).〕〔(www.scientificamerican.com Dark Matter May Feel a “Dark Force” That the Rest of the Universe Does Not )〕〔(Monthly Notices of the Royal Astronomical Society Volume 449 Issue 4Pp. 3393-3406 The behaviour of dark matter associated with four bright cluster galaxies in the 10 kpc core of Abell 3827 ) 〕 ==References==
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