Papers discussed: {#papers_discussed}¶
https://arxiv.org/abs/1609.08626 : Study of the impact of halo
contraction due to the baryonic potential on CDM versus SIDM haloes of
different sizes (Dwarf galaxies, LSB, Elliptical, Clusters). The result
depend on halo masses and on the assumed baryon potential. SIDM haloes
can even collapse for a steep baryon profile.