
This 3D map illustrates the large-scale distribution of dark matter, reconstructed from measurements of weak gravitational lensing by using the Hubble Space Telescope. Credit: Image courtesy of DOE/Lawrence Livermore National Laboratory
Lattice Strong Dynamics Collaboration, led by a Lawrence Livermore National Lab team, has combined theoretical and computational physics techniques and used the Laboratory’s massively parallel 2-petaflop Vulcan supercomputer to devise a new model of dark matter. It identifies it as naturally “stealthy” today, but would have been easy to see via interactions with ordinary matter in the extremely high-temperature plasma conditions that pervaded the early universe.
Dark matter makes up 83% of all matter in the universe and does not interact directly with elect...
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![The magnetic field of the O-type star called NGC 1624-2 is unusually large for its class. Credit: SOHO/[instrument] Consortium. SOHO is a project of international cooperation between ESA and NASA. The magnetic field of the O-type star called NGC 1624-2 is unusually large for its class. Credit: SOHO/[instrument] Consortium. SOHO is a project of international cooperation between ESA and NASA.](https://images.sciencedaily.com/2015/09/150923082607_1_540x360.jpg)

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