Researchers in the U.S. have carried out the most stringent tests to date of the idea that an ultraviolet glow in the atmospheres of giant p
Researchers in the U.S. have carried out the most stringent tests to date of the idea that an ultraviolet glow in the atmospheres of giant planets could partly arise through the indirect interaction between dark matter and ordinary matter. Led by Carlos Blanco at Penn State University and Rebecca Leane at the SLAC National Accelerator Laboratory, the team's results place some of the tightest constraints yet on the strength of this interaction. Published in Physical Review Letters, the study also strengthens the possibility that the giant planets in our solar system could be used as natural dark matter detectors.
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