Computer Science
Scientific paper
Aug 2010
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aipc.1274...97n&link_type=abstract
AXIONS 2010: Proceedings of the International Conference. AIP Conference Proceedings, Volume 1274, pp. 97-102 (2010).
Computer Science
Dark Matter, Galaxies, Symmetry Breaking, Baryon Mass, Dark Matter, Galactic Halo, Spontaneous And Radiative Symmetry Breaking, Baryons
Scientific paper
The continuous infall of dark matter with low velocity dispersion in galactic halos leads to the formation of high density structures called caustics. Dark matter caustics are of two kinds : outer and inner. Outer caustics are thin spherical shells surrounding galaxies while inner caustics have a more complicated structure that depends on the dark matter angular momentum distribution. The presence of a dark matter caustic in the plane of the galaxy modifies the gas density in its neighborhood which may lead to observable effects. Caustics are also relevant to direct and indirect dark matter searches.
No associations
LandOfFree
Dark Matter Caustics does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Dark Matter Caustics, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Dark Matter Caustics will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1862825