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Self-interacting dark matter and small-scale gravitational lenses in galaxy clusters

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This article is published in Physical Review D.The article was published on 2021-11-29 and is currently open access. It has received 9 citations till now. The article focuses on the topics: Self-interacting dark matter & Scale (ratio).

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Snowmass2021 Theory Frontier White Paper: Astrophysical and Cosmological Probes of Dark Matter

TL;DR: In this article , a more comprehensive understanding of dark matter within the next decade will require overcoming a number of theoretical challenges: the groundwork for these strides is being laid now, yet much remains to be done.
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Gravothermal evolution of dark matter halos with differential elastic scattering

TL;DR: In this paper , the authors study the gravothermal evolution of dark matter halos in the presence of differential self-scattering that has strong velocity and angular dependencies and show that the three moments of the Boltzmann equation under the fluid approximation are satisfied.
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Dynamical instability of collapsed dark matter halos

TL;DR: In this article , a truncated Maxwell-Boltzmann distribution is used to model the dark matter distribution and solve the Tolman-Oppenheimer-Volkoff equation.
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Discriminating power of milli-lensing observations for dark matter models

TL;DR: In this paper , the authors investigate the ability of sub-galactic DM haloes to act as strong lenses on background compact sources, producing gravi- tational lensing events on milli-arcsecond scales (milli-lenses), for different DM models.
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Constraining resonant dark matter self-interactions with strong gravitational lenses

- 04 May 2023 - 
TL;DR: In this article , a method to constrain self-interacting dark matter (SIDM) from observations of quadruply imaged quasars, and apply it to five selfinteraction potentials with a long-range dark force was devised.
References
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Journal ArticleDOI

A Universal Density Profile from Hierarchical Clustering

TL;DR: In this article, the authors used high-resolution N-body simulations to study the equilibrium density profiles of dark matter halos in hierarchically clustering universes, and they found that all such profiles have the same shape, independent of the halo mass, the initial density fluctuation spectrum, and the values of the cosmological parameters.
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Planck 2013 results. XVI. Cosmological parameters

Peter A. R. Ade, +327 more
TL;DR: In this paper, the authors present the first cosmological results based on Planck measurements of the cosmic microwave background (CMB) temperature and lensing-potential power spectra, which are extremely well described by the standard spatially-flat six-parameter ΛCDM cosmology with a power-law spectrum of adiabatic scalar perturbations.
Journal ArticleDOI

Planck 2013 results. XVI. Cosmological parameters

Peter A. R. Ade, +262 more
TL;DR: In this paper, the authors present the first results based on Planck measurements of the CMB temperature and lensing-potential power spectra, which are extremely well described by the standard spatially-flat six-parameter LCDM cosmology.
Journal ArticleDOI

The Cosmological simulation code GADGET-2

TL;DR: GADGET-2 as mentioned in this paper is a massively parallel tree-SPH code, capable of following a collisionless fluid with the N-body method, and an ideal gas by means of smoothed particle hydrodynamics.
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Introducing the Illustris Project: simulating the coevolution of dark and visible matter in the Universe

TL;DR: The Illustris Project as mentioned in this paper is a series of large-scale hydrodynamical simulations of galaxy formation, which includes primordial and metal-line cooling with self-shielding corrections, stellar evolution, stellar feedback, gas recycling, chemical enrichment, supermassive black hole growth, and feedback from active galactic nuclei.