Page 20 - EUREKA! Fall 2017
P. 20

Dark matter is by far the dominant stuff in


                the universe, and we still have essentially no
                clue what it is.










        before they can solve a mystery that   liked about it,” he says, “is that you’re   the world are currently on the hunt
        has been confounding physicists for   required to understand some fairly   for dark matter, including work at the            Caption: top, below left, right
        decades, Boulay and his collaborators   simple concepts but there’s very little   Large Hadron Collider near Geneva,         etc Sustrum facea pa cus non
                                                                                                                                     et fugit explat offictatia simus
        — a group of more than 75 researchers   memorization, which I was never   the LUX underground experiment in                  pedi aliatec totati quatus
        from 10 institutions in Canada, the   very good at. So I always excelled in   South Dakota, the XMASS project at             solorerro dicil explit, nonse
        U.K. and Mexico — must first address   physics, because once you understand   Japan’s Kamioka Observatory, and               se endem iuritae preprorias
        a seemingly endless string of details.   a few basic concepts you can go a   the IceCube Neutrino Observatory, a             asi blatur si temposs itatur,
        Today, up on that ladder, four months   long way.”                       particle detector at the South Pole.                toreribus rerrovitem quunt, si
                                                                                                                                     tem ius, sende nisitincia cuptas
        after the experiment was first fired   Boulay earned an undergraduate    But DEAP, which was conceived of                    eaque venditatus volenis
        up in November 2016, Boulay and      degree in physics at Laurentian     around 2004, when Boulay was doing                  moloresto int.                                                                                            Photo: Luther Caverly
        SNOLAB operations supervisor Tony    University in Sudbury when the      a post-doc at the Los Alamos National
        Flower are trying to figure out how   Sudbury Neutrino Observatory       Laboratory in New Mexico, represents
        to fix a bug in the cryogenic system.   experiment was starting, exposing   perhaps the best shot scientists have.
        When it runs, as it is expected to   him to particle physics, and stayed at   Its potential is rooted in the unique
        do for years, it vibrates, and that   Laurentian for his master’s degree. He   properties of argon, which will help
        movement appears to be damaging      got involved in the final assembly of   researchers discriminate backgrounds
        and loosening some of its components   the SNO detector (see “SNO story,”   when they study the recoil of
        and fittings.                        page TK) while working toward his   scattering particles, as well as the large
          “This is typically of the lower-level   PhD at Queen’s University, and had an   volume of argon being deployed. Every
        mechanical problems we’re sorting    opportunity to analyze its first results.   other component of the detector has
        out,” says Boulay, DEAP’s project    Then he zeroed in on the quest for   an extremely low level of radioactivity,
        director and a Canada Research Chair   dark matter.                      which will allow the experiment
        in Particle Astrophysics and Subatomic   The term “dark matter” was coined   to capitalize on the sensitivity of
        Physics. “We’re certainly dealing with   in the 1930s by Swiss astronomer   its location deep underground at
        a lot of technical and engineering   Fritz Zwicky, who, according to the   SNOLAB.
        challenges, but the concept of a     DEAP website, “determined the mass
        particle scattering off a nucleus like a   and velocity distributions of objects   In 2006, Boulay led the development
        billiard ball is fairly straightforward. At   within the Coma galaxy cluster, and   of a small prototype detector with
        a fundamental level, what we’re doing   found that the velocity distributions he   liquid argon at Queen’s to demonstrate
        is pretty simple, yet it’s one of the   calculated implied the cluster had much   that this process could work. That
        biggest questions in particle physics,   more mass than the observable light   design, and expertise from the SNO
        and maybe in science.                suggested.” Forty years later, American   experiment, informed the construction
          “This is by far the dominant stuff   astronomer Vera Rubin corroborated   of the full-scale version. The argon
        in the universe,” he says about dark   the existence of dark matter by   vessel, which has an inner radius of
        matter, “and we still have essentially no   studying the rotation of galaxies and   85 centimetres, is surrounded by
        clue what it is.”                    concluding they “rotated too fast for   255 photomultiplier tubes (PMTs) to
                                             the gravitational force of their visible   capture the light pulses, and the whole
        In a sense, Boulay was destined to   stars to hold them together.” Her   apparatus is immersed in a water tank
        lead DEAP. He was born and raised    results “pointed to the existence of vast   to further block external radiation.
        in Sturgeon Falls, an hour east      amounts of unobservable mass, even   Since it was turned on last November,
        of Sudbury on the Trans-Canada       10 times more than visible, surrounding   much of the focus at DEAP has been
        Highway, and became interested in    galaxies of stars.”                 calibrating the detector and collecting
        physics at a young age. “The thing I   Several dozen experiments around                   (continued on page 23)



        20  science.carleton.ca                                                                                                                                                  Photo:                                   science.carleton.ca  21  Photo:
   15   16   17   18   19   20   21   22   23   24   25