LUX Dark Matter Search
November 20, 2013
I received my undergraduate physics degree during the dark days of physics funding at the start of the 1970s. At that time, US government funding of science had been stagnant for many years, and it would continue to be stagnant for years to come (see figure). This was a consequence of the Vietnam War, which drained both the country's wallet, and its spirit.
Although I was a physicist, I had always enjoyed engineering research, and I tried finding a suitable job in that area after graduation. Alas, none could be found, so I did what many unemployed graduates do today, I went to graduate school. I had read in articles in economics journals that the real purpose of college was not to educate, but to keep people out of the job market for four years. Suddenly, the purpose of graduate school was to keep educated people out of the job market for a few additional years.
Graduate school was different, too. I could get a research assistantship in materials science, but not in physics, so that's how I became a materials scientist. Shakespeare's phrase, "A rose by any other name...," is actually true. In the end, my solid state physics colleagues and I had taken equivalent courses, sometimes siting in the same classrooms; and, we were doing similar experiments, and graduated to compete for the same jobs.
Those dark days of physics are long past, and now there's the brighter darkness of well funded experiments for elucidating dark dark matter. As I wrote in a previous article (Whither WIMPs, November 22, 2010), about 80% of the mass of the universe is supposed to consist of weakly interacting massive particles (WIMPs). These particles, invisible because they do not interact electromagnetically, only gravitationally, are the supposed components of dark matter.
One way to detect this sort of particle is to monitor a huge quantity of an indicator material of large nuclei and hope for an interaction. This approach has been ongoing in the XENON Dark Matter Search Experiment, which uses a vat of liquid xenon as the detector. Interaction between a WIMP and xenon will produce both a scintillation and an ionization, so a WIMP interaction will have a particular interaction "signature."
Xenon (atomic number 54) has many stable isotopes with nuclei that contain 70 or more neutrons, so there's hope for some interaction. One problem is distinguishing a dark matter interaction from others caused by background sources, such as cosmic rays and local radioactive sources. WIMP interaction with normal matter has been estimated to be anywhere from a single event per kilogram per year to a single event per ton per year.
The XENON Dark Matter Search Experiment operates at the Gran Sasso Underground Laboratory (Laboratori Nazionali del Gran Sasso) in Italy, where it's protected from most cosmic radiation. This experiment has not detected any WIMPs over several years of operation. However, no result is still a result in that it places a limit on what a WIMP might be. At this point, The cross-section of the WIMP-nucleon interaction is about 10-45 cm2.
The XENON Dark Matter Search Experiment isn't the only xenon-based experiment in search of WIMPs. There's also the Large Underground Xenon Detector (LUX).[3-13] Like the XENON Dark Matter Search Experiment, LUX is located in an underground laboratory, the Sanford Underground Laboratory, built into an abandoned mile-deep gold mine in Lead, South Dakota. LUX has several times more liquid xenon than the XENON Dark Matter Search Experiment.
The key to such an experiment is reduction in background signals. Aside from it's being located in a cavern 4,850 feet underground, the detector is surrounded by 70,000 gallons of water, and it's made from titanium and Teflon, which have no natural radioactivity.[4,10] The cavern is the same place where Raymond Davis, Jr., winner of the 2002 Nobel Prize in Physics, detected solar neutrinos using a container filled with 100,000 gallons of the common dry-cleaning chemical, tetrachloroethylene as a detector.[5,10,12] I wrote about the Davis experiment in a previous article (Bacterial Iron Isotopes, July 22, 2013).
LUX is funded by the US National Science Foundation and the United States Department of Energy. The Sanford Lab is owned by South Dakota, which is one way to stimulate the local economy, and it was made possible through a a $70 million donation by philanthropist T. Denny Sanford. Lux is a huge scientific collaboration involving seventeen research universities and national laboratories in the United States, the United Kingdom, Portugal, and Russia; so the result of its first, 85-day experiment, has gotten a lot of press coverage.[4-13] This is all the more interesting, since what was reported at an October 30, 2013, webcast was a null result.
Yale University physicist, Daniel McKinsey, who is on the LUX team, is quoted in Wired as saying, "Basically, we saw nothing. But we saw nothing better than anyone else so far."
The LUX detector was filled with liquid xenon in February of this year, and it completed a baseline run of 85 days during the summer, followed by data analysis. There were 160 detected events, and all of these were determined to have been produced by background radiation, and not by WIMPs.[4-5,7,13] This result rules out some supposed positive events seen at other experiments.
LUX is twice as sensitive to heavy WIMPs than XENON, but it's nearly twenty times more sensitive to WIMPs of low mass. For this reason, these data seem to rule-out models for WIMPs in the 33 GeV mass range. Specifically rejected are early claims of WIMP detection by three other experiments, DAMA (DArk MAtter), the Cryogenic Dark Matter Search (CDMS), and the Coherent Germanium Neutrino Technology (CoGeNT). CoGeNT had reported a WIMP in the 7-11 GeV mass range, and the other two experiments had offered candidates as well.[2,11]
LUX is scheduled for a 300 day run in 2014, and the experiment will continue in this form for two years.[4,5] As LUX runs over longer periods, the chance for a dark matter discovery will increase. After LUX, the research team is hoping to obtain funding to scale the experiment to seven tons of xenon in a device called LUX-ZEPLIN (LZ). LUX-ZEPLIN will have 100 times the LUX sensitivity.[2,5,7,9] At that point, not detecting WIMPs will have everyone scratching their heads.
|The end of the 1960s, and the start of the 1970s, was a bad time for science in the United States.|
(National Science Foundation data from ref. 1, graphed using Gnumeric.)
- Federal obligations for research and development, 1951-2002, National Science Foundation Web Site (XL Spreadsheet).
- Editors' Choice: All Quiet on the Dark Front, Science, vol. 330, no. 6004 (October 29, 2010), p. 563.
- Large Underground Xenon dark matter experiment web site.
- First results from LUX dark matter detector, Brown University Press Release, October 30, 2013.
- First results from LUX dark matter detector rule out some candidates, University of California, Davis, Press Release, October 30, 2013.
- First Results from World's Most Sensitive Dark Matter Detector Announced, University of Rochester Press Release, October 30, 2013.
- Eugenie Samuel Reich, "No sign of dark matter in underground experiment," Nature, October 30, 2013.
- Rebecca Morelle, LUX results: Dark matter hunt nears final phase, BBC World Service, October 30, 2013.
- Simon Levey, "New dark matter detector sends first data from gold mine 1.5 km underground," Imperial College Press Release, October 30, 2013.
- Adam Mann, "Huge Dark Matter Experiment Finds Nothing but More Mysteries," Wired, October 30, 2013.
- Clara Moskowitz, "Dark Matter Still Hiding: Latest Experimental Sweep Comes Up Empty," Scientific American, October 30, 2013.
- Dennis Overbye, "Dark Matter Experiment Has Found Nothing, Scientists Say Proudly," The New York Times, October 30, 2013.
- Richard Chirgwin, "Dark matter: We have found simply NOTHING, crow physicists," The Register (UK), October 31, 2013.
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