April 16, 2013 report
Super-CDMS researchers report possible evidence of WIMPs
Researchers in several facilities around the world (and aboard the International Space Station) are looking for evidence of WIMPs, because theory suggests that they constitute dark matter, the invisible material believed to make up approximately 85 percent of all matter that exists in the universe. Because WIMPs can't be seen directly, researchers look to events that might prove they exist, such as collisions between WIMPs and atomic nuclei. In order to find such evidence, researchers set up detectors they hope will catch such collisions that occur due to gravitational pull on WIMPs—they are believed to interact only rarely with normal matter through other means.
Researchers at the Super-CDMS facility have set up eight silicon detectors (cooled to -459.67 degrees Fahrenheit) in the hope of detecting the slight amount of heat given off by a collision between a WIMP and an atom's nucleus. The researchers report detection of three events that might have been the result of such collisions, though they are quick to add that the events might also have been due to something else, such as statistical errors. However, calculations indicate the events are 99.81 percent more likely to be WIMPs than background fluctuations, which translates to approximately a three-sigma level of confidence.
Interestingly, if the detected events do turn out to be the result of WIMP/nucleus collisions, it will mean that WIMPs are much lighter than scientists have been expecting—the detected collisions detected to just 8.6 giga-electronvolts. The researchers note this finding is in line with results from other research efforts, though they also acknowledge that it contradicts the findings of other researchers. Regardless, research at the Super-CDMS facility and elsewhere will continue until WIMP collisions are proven to exist, or not.
Silicon Detector Results from the First Five-Tower Run of CDMS II. arXiv astro-ph.CO, (2013), arXiv:1304.3706
E. Figueroa-Feliciano's presentation at Light Dark Matter 2013.
© 2013 Phys.org