Mapping dark matter

July 24, 2017, Harvard-Smithsonian Center for Astrophysics
Abell 2744, a cluster of galaxies whose dark matter halo has imaged more distant galaxies as seen in this Hubble Space Telescope image. Astronomers have compared the image to simulations of dark matter lensing and found excellent agreement, indicating that that current models of dark matter behavior on the large scale are quite good. Credit: NASA/ESA/Hubble

About eighty-five percent of the matter in the universe is in the form of dark matter, whose nature remains a mystery. The rest of the matter in the universe is of the kind found in atoms. Astronomers studying the evolution of galaxies in the universe find that dark matter exhibits gravity and, because it is so abundant, it dominates the formation of large-scale structures in the universe like clusters of galaxies. Dark matter is hard to observe directly, needless to say, and it shows no evidence of interacting with itself or other matter other than via gravity, but fortunately it can be traced by modeling sensitive observations of the distributions of galaxies across a range of scales.

Galaxies generally reside at the centers of vast clumps of called haloes because they surround the clusters of galaxies. Gravitational lensing of more distant galaxies by dark matter haloes offers a particularly unique and powerful probe of the detailed distribution of dark matter. So-called strong creates highly distorted, magnified and occasionally multiple images of a single source; so-called weak lensing results in modestly yet systematically deformed shapes of background galaxies that can also provide robust constraints on the distribution of dark matter within the clusters.

CfA astronomers Annalisa Pillepich and Lars Hernquist and their colleagues compared gravitationally distorted Hubble images of the galaxy cluster Abell 2744 and two other clusters with the results of computer simulations of dark matter haloes. They found, in agreement with key predictions in the conventional dark matter picture, that the detailed galaxy substructures depend on the distribution, and that the total mass and the light trace each other. They also found a few discrepancies: the radial distribution of the dark matter is different from that predicted by the simulations, and the effects of tidal stripping and friction in are smaller than expected, but they suggest these issues might be resolved with more precise simulations. Overall, however, the standard model of dark matter does an excellent and reassuring job of describing galaxy clustering.

Explore further: Team puts dark matter on the map

More information: Priyamvada Natarajan et al. Mapping substructure in the HST Frontier Fields cluster lenses and in cosmological simulations, Monthly Notices of the Royal Astronomical Society (2017). DOI: 10.1093/mnras/stw3385

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RNP
5 / 5 (3) Jul 24, 2017
A link to open access copy of the paper can be found here; https://arxiv.org...02.04348
cantdrive85
1 / 5 (5) Jul 24, 2017
Thanks DNP, I needed a laugh today. There certainly is no shortage of these pseudo-sci-fi peer reviewed papers floating around out there.
Captain Stumpy
5 / 5 (3) Jul 24, 2017
@nazi sympathizing pseudoscience eu cult idiot

if it's pseudoscience and obviously you know better because evidence

then why haven't you been able to publish a refute to the studies you claim are pseudoscience?

did bigfoot steal your theory ?
http://journals.p....0075637

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