On the fraction of dark matter in charged massive particles (CHAMPs) [PDF]
, 2010 From various cosmological, astrophysical and terrestrial requirements, we derive conservative upper bounds on the present-day fraction of the mass of the Galactic dark matter (DM) halo in charged massive particles (CHAMPs). If dark matter particles are neutral but decay lately into CHAMPs, the lack of detection of heavy hydrogen in sea water and the ...
arxiv +1 more source
Dark matter halo mass functions and density profiles from mass and energy cascade. [PDF]
Sci Rep, 2023 Xu ZJ.
europepmc +1 more source
Universal scaling laws and density slopes for dark matter haloes. [PDF]
Sci Rep, 2023 Xu Z.
europepmc +1 more source
The structure of halos in Self-Interacting Cold Dark Matter models [PDF]
Rev.Mex.Astron.Astrofis. 17 (2003) 19, 2003 High-resolution numerical simulations were performed to study the structure and substructure of Milky Way- and cluster-sized halos in a LCDM cosmology with self-interacting (SI) dark particles, where the particle cross section, +AFw-sig, is assumed constant or inversely proportional to the relative velocity.
arxiv
Cosmic ray feedback in galaxies and galaxy clusters: A pedagogical introduction and a topical review of the acceleration, transport, observables, and dynamical impact of cosmic rays. [PDF]
Astron Astrophys Rev, 2023 Ruszkowski M, Pfrommer C.
europepmc +1 more source
Galactic constraints on CHAMPs [PDF]
arXiv, 2008 We improve earlier Galactic bounds that can be placed on the fraction of dark matter in charged elemental particles (CHAMPs). These constraints are of interest for CHAMPs whose mass is too large for them to have seen through their electromagnetic interaction with ordinary matter, and whose gyroradius in the galactic magnetic field is too small for halo
arxiv
Preservation of Cuspy Profiles in Disk Galaxy Mergers [PDF]
arXiv, 2005 We carried out three self-consistent $N$-body simulations of galaxy mergers, with a cuspy dark matter profile, in order to study if the inner dark density slope is preserved in the remnants. In these simulations the progenitors include both a stellar disk and an intrinsic angular momentum for the halos, unlike previous similar studies.
arxiv
SIDM on FIRE: hydrodynamical self-interacting dark matter simulations of low-mass dwarf galaxies. [PDF]
Mon Not R Astron Soc, 2017 Robles VH +9 more
europepmc +1 more source
Cold dark matter: Controversies on small scales. [PDF]
Proc Natl Acad Sci U S A, 2015 Weinberg DH +4 more
europepmc +1 more source
Galaxy formation with BECDM - I. Turbulence and relaxation of idealized haloes. [PDF]
Mon Not R Astron Soc, 2017 Mocz P +6 more
europepmc +1 more source