Astronomy and Astrophysics – Astrophysics
Scientific paper
2000-03-31
Astrophys.J.543:514,2000
Astronomy and Astrophysics
Astrophysics
submitted to ApJ
Scientific paper
10.1086/317149
We study the evolution of Hernquist profile ``galaxies'' in the presence of self-interacting dark matter (SIDM), where the properties of the dark matter can be parameterized by one number, sigma-hat = sigma M/a^2 for a halo of mass M and break radius a. While the halos form constant density cores of size a/2 on the core radius relaxation time scale core collapse begins shortly thereafter and a steeper 1/r^2 central density cusp starts forming faster than predicted by 2-body relaxation. The formation of the steeper central cusp is accelerated if the cooling baryons adiabatically compress the dark matter. The natural consequence of SIDM is to exacerbate rather than to mitigate astrophysical problems created by dark matter density cusps.
Kochanek Chris S.
White Martin
No associations
LandOfFree
A Quantitative Study of Interacting Dark Matter in Halos 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 A Quantitative Study of Interacting Dark Matter in Halos, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and A Quantitative Study of Interacting Dark Matter in Halos will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-290970