Effective cross section of fuzzy dark matter halos
@article{Bak2020EffectiveCS, title={Effective cross section of fuzzy dark matter halos}, author={Dongsu Bak and Jae-weon Lee and Sangnam Park}, journal={Journal of the Korean Physical Society}, year={2020}, volume={79}, pages={582 - 588} }
We numerically study the movement of two colliding fuzzy dark matter solitons without explicit self-interaction and find the effective cross section of dissipative change in velocity. The cross section turns out to be inversely proportional to the velocity cubed, and we present its analytic interpretation. Using the result we roughly estimate spatial offsets during head-on collisions of two fuzzy dark matter halos, which can be related to the spatial offsets between stars and dark matter in…
2 Citations
Analyzing planar galactic halo distributions with fuzzy/cold dark matter models
- PhysicsJournal of Cosmology and Astroparticle Physics
- 2022
We perform a numerical comparison between the fuzzy dark matter model and the cold dark matter model, focusing on formation of satellite galaxy planes around massive galaxies. Such galactic dynamics…
Probing ultra-light axion dark matter from 21 cm tomography using Convolutional Neural Networks
- PhysicsJournal of Cosmology and Astroparticle Physics
- 2022
We present forecasts on the detectability of Ultra-light axion-like particles (ULAP) from future 21 cm radio observations around the epoch of reionization (EoR). We show that the axion as the…
References
SHOWING 1-10 OF 31 REFERENCES
The nongravitational interactions of dark matter in colliding galaxy clusters
- PhysicsScience
- 2015
Combining these measurements statistically, the existence of dark mass is detected at 7.6σ significance, implying a self-interaction cross section σDM/m < 0.47 cm2/g (95% CL) and disfavoring some proposed extensions to the standard model.
Brief History of Ultra-light Scalar Dark Matter Models
- Physics
- 2018
This is a review on the brief history of the scalar field dark matter model also known as fuzzy dark matter, BEC dark matter, wave dark matter, or ultra-light axion. In this model ultra-light scalar…
Merger of galactic cores made of ultralight bosonic dark matter
- PhysicsRevista Mexicana de Física
- 2021
We study binary mergers of ultralight bosonic dark matter cores by solving the Gross-Pitaevskii- Poisson system of equations. The analysis centers on the dynamics of the relaxation process and the…
Behavior of luminous matter in the head-on encounter of two ultralight BEC dark matter halos
- Physics
- 2016
Within the context of ultralight BEC dark matter, we analyze the head-on encounters of two structures. These structures are made of a BEC component, which is a ground state equilibrium solution of…
Gravitational Cooling of Self-gravitating Bose Condensates
- Physics
- 2006
Equilibrium configurations for a self-gravitating scalar field with self-interaction are constructed. The corresponding Schrödinger-Poisson (SP) system is solved using finite differences, assuming…
A Direct Empirical Proof of the Existence of Dark Matter
- Physics
- 2006
We present new weak-lensing observations of 1E 0657-558 (z = 0.296), a unique cluster merger, that enable a direct detection of dark matter, independent of assumptions regarding the nature of the…
The Structure of cold dark matter halos
- Physics
- 1996
High resolution N-body simulations show that the density profiles of dark matter halos formed in the standard CDM cosmogony can be fit accurately by scaling a simple “universal” profile. Regardless…
Ultralight scalars as cosmological dark matter
- Physics
- 2017
Many aspects of the large-scale structure of the Universe can be described successfully using cosmological models in which 27±1% of the critical mass-energy density consists of cold dark matter…