Supermassive Black Holes from Ultra-Strongly Self-Interacting Dark Matter
@article{Pollack2014SupermassiveBH, title={Supermassive Black Holes from Ultra-Strongly Self-Interacting Dark Matter}, author={Jason Pollack and David N. Spergel and Paul J. Steinhardt}, journal={arXiv: Cosmology and Nongalactic Astrophysics}, year={2014} }
We consider the cosmological consequences if a small fraction ($f\lesssim 0.1$) of the dark matter is ultra-strongly self-interacting, with an elastic self-interaction cross-section per unit mass $\sigma\gg1\ \mathrm{cm^{2}/g}$. This possibility evades all current constraints that assume that the self-interacting component makes up the majority of the dark matter. Nevertheless, even a small fraction of ultra-strongly self-interacting dark matter (uSIDM) can have observable consequences on…
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References
SHOWING 1-10 OF 120 REFERENCES
Observational Constraints on the Self-interacting Dark Matter Scenario and the Growth of Supermassive Black Holes
- Physics
- 2001
We consider the astrophysical consequences of the self-interacting dark matter (SIDM) scenario for a general velocity-dependent cross section per unit mass that varies as some power of velocity: σDM…
Constraining self-interacting dark matter with the Milky Way’s dwarf spheroidals
- Physics
- 2013
Self-Interacting Dark Matter is an attractive alternative to the Cold Dark Matter paradigm only if it is able to substantially reduce the central densities of dwarf-size haloes while keeping the…
Subhaloes in self-interacting galactic dark matter haloes
- Physics
- 2012
We present N-body simulations of a new class of self-interacting dark matter models, which do not violate any astrophysical constraints due to a non-power-law velocity dependence of the transfer…
Cosmological simulations with self-interacting dark matter – II. Halo shapes versus observations
- Physics
- 2013
If dark matter has a large self-interaction scattering cross section, then interactions among dark-matter particles will drive galaxy and cluster halos to become spherical in their centers. Work in…
Self-interacting dark matter
- Physics
- 1992
A new type of dark matter is considered. As with cold dark matter, when the dark matter is nonrelativistic, it does not couple to the electron-photon plasma, so its entropy per comoving volume is…
Weakly Self-interacting Dark Matter and the Structure of Dark Halos
- Physics
- 2000
We study the formation of dark halos in a ΛCDM universe under the assumption that cold dark matter (CDM) particles have a finite cross section for elastic collisions. We compare evolution when CDM…
Self-Interacting Dark Matter Halos and the Gravothermal Catastrophe
- Physics
- 2002
We study the evolution of an isolated spherical halo of self-interacting dark matter (SIDM) in the gravothermal fluid formalism. We show that the thermal relaxation time tr of an SIDM halo with the…
Cosmological Simulations with Self-Interacting Dark Matter I: Constant Density Cores and Substructure
- Physics
- 2013
We use cosmological simulations to study the effects of self-interacting dark matter (SIDM) on the density profiles and substructure counts of dark matte r halos from the scales of spiral galaxies to…
Forming supermassive black holes by accreting dark and baryon matter
- Physics
- 2005
Given a large-scale mixture of self-interacting dark matter (SIDM) particles and baryon matter distributed in the early Universe, we advance here a two-phase accretion scenario for forming…