Masao Mori, Astrophysics, University of Tsukuba
Theoretical Astrophysics and Computational Physics

Dark matter haloes · 2014 · Journal article

Can cusp-to-core transformation connect common dwarf-halo masses and surface densities?

An analytical transformation model connects two reported regularities of low-mass dark matter haloes.

The connection between the cusp-to-core transformation and observational universalities of DM haloes

The connection between the cusp-to-core transformation and observational universalities of DM haloes. Ogiya, Go; Mori, Masao; Ishiyama, Tomoaki; Burkert, Andreas, Monthly Notices of the Royal Astronomical Society: Letters, 440, L71–L75 (2014).

Approach

The study tests whether converting initially cuspy haloes to cores can reproduce the near-common central surface density and mass enclosed within 300 parsecs.

Main result

The transformation model recovers the surface-density relation; the common enclosed mass follows within the dwarf-galaxy regime. Core densities also carry information about formation epochs.

Scientific implications

The work connects halo regularities to structural evolution rather than treating each empirical relation as independent.

Scope and limitations

These are consequences of the transformation assumptions and the observational relations considered, not proof of one specific feedback mechanism.

Related papers

Browse all research briefings · Publication list

Research summaries prepared with AI assistance from the linked papers and abstracts. Consult the original publications for full methods and results.

Updated · Contact