Welcome to the DarkSide: Project aims to find particles of dark matter

Jan 17, 2014 by Catherine Zandonella
Welcome to the DarkSide: Project aims to find particles of dark matter
The DarkSide-50 research team is made up of faculty, students and researchers from dozens of institutions around the world, including, from left, Luca Grandi, an assistant professor at the University of Chicago, Richard Saldanha, an associate fellow in the Kavli Institute for Cosmological Physics at the University of Chicago, and Hanguo Wang, a researcher at the University of California-Los Angeles. While wearing protective clothing to keep the environment clean, they are working to assemble the core of the dark matter detector, an argon-filled tank with photodetectors at the top and bottom to spot the light from collisions, and copper coils to help determine where the collisions occur. Credit: Peter Meyers

(Phys.org) —In a laboratory under a mountain 80 miles east of Rome this fall, a Princeton-led international team switched on a new experiment aimed at finding a mysterious substance that makes up a quarter of the universe but has never been seen.

The experiment, known as DarkSide-50, is searching for particles of dark matter. For the last several decades, researchers have known that visible matter—the stuff we can see—makes up only 4 percent of the universe, while dark energy is thought to make up about 73 percent. Dark matter is thought to make up the remaining 23 percent, and finding it, researchers say, will solidify our understanding of how the universe formed and shed light on its ultimate fate.

"This is like the search for the Higgs boson was 10 years ago," said Peter Meyers, a professor of physics at Princeton University and one of the lead scientists on the project. "We have a good idea of what to look for, but we don't know exactly where or when we will find it."

Housed inside a cavernous chamber in Italy's Gran Sasso National Laboratory, the DarkSide-50 collaboration involves 17 American institutions as well the Italian Institute for Nuclear Physics and other institutions in Italy, France, Poland, Ukraine, Russia and China. The research team includes postdocs, staff researchers and several graduate and undergraduate students from Princeton.

The researchers spent last summer assembling the detector, which consists of three fluid-filled chambers nested one inside the other like Russian dolls. Now that the experiment is up and running, the waiting begins. Unlike the massive Large Hadron Collider that discovered the Higgs, DarkSide-50 doesn't smash anything. Instead, it is designed to detect that drift through its chambers.

Looking for WIMPs

The evidence for dark matter dates to the 1930s, when astronomers realized that the amount of matter we can see—as planets, stars and galaxies—falls far short of what must be out there to give galaxies their characteristic spiral shapes and clustering patterns.

Without this missing matter, the galaxies should have flown apart long ago. Matter provides the gravity that keeps the stars in rotation around the galaxy's center. Unless our theories of gravity are wrong—and a minority of physicists think that is a possibility—dark matter must exist.

"Finding dark matter particles would help confirm our understanding of the universe," said Cristiano Galbiati, an associate professor of physics at Princeton. "And, whether or not we find it, we will have learned a great deal about how to go about looking for it. This is as exciting a moment in the search for dark matter as there has ever been."

Although no one knows for sure what dark matter is made of, the DarkSide-50 team and many other scientists think the most likely candidate is a particle so weak that it is called a WIMP, which is short for "weakly interacting massive particle."

As the name suggests, WIMPs barely interact with their surroundings. They simply drift through walls like ghosts. If you cup your hands together, you will surround—but never trap—a few of these ethereal beings.

Scientists suggest that a WIMP can be detected when it smacks into the nucleus of an atom such as argon, which is found in air. When this happens in a chamber of densely packed argon atoms, the stricken atom recoils and creates a track of excited argon atoms in its wake. This track appears as a fleeting trail of light, which can be detected by devices called photodetectors.

But these collisions are rare—just a few WIMPs are detected each year. Because other particles also give off light when they collide with argon, DarkSide-50 is located nearly a mile beneath Gran Sasso mountain ("gran sasso" is Italian for "great stone"). The rock shields out cosmic-ray particles that routinely bombard the Earth.

"Separating the rare WIMP events from background is the main challenge of all dark matter experiments," said Princeton physics professor Frank Calaprice, who leads the project with Meyers and Galbiati.

"DarkSide is an attempt to build an apparatus that is as close as possible to an ideal 'background-free detector.' The design benefits from methods and two decades of experience that the Princeton group had developing the Borexino solar neutrino experiment," he said, referring to another experiment at Gran Sasso that ultimately achieved record-breaking low backgrounds and the detection of rare solar neutrinos, which are elementary particles that were theorized to exist long before they were detected.

The scientists and students from Princeton and the other institutions have spent hours in this secluded laboratory, which is accessible solely from an exit off a six-mile-long tunnel on a highway that traverses Italy from Rome to the country's east coast. Vehicles approaching the lab are stopped by a large steel door and guard station, prompting comparisons to a supervillain's lair.

The DarkSide-50 experiment is in progress at Gran Sasso National Laboratory in central Italy, located nearly a mile beneath Gran Sasso mountain so that the rock can shield the detector from cosmic-ray particles. Researchers stay in the town of Assergi, shown above, when they are working on the project. Credit: Will Taylor

The project exemplifies why Princeton is an exceptional place to study as an undergraduate, said senior Will Taylor, who spent a week at the lab in October working on a system for removing trace amounts of radioactive particles from the water used in the detector.

"What makes Princeton special," Taylor said, "is that if you see a professor's door open, you can walk in and ask to join an experiment. And this is one of the most sophisticated experiments in the world."

Prepping for supersensitive testing

DarkSide-50 is located in one of three caverns at Gran Sasso. The WIMP detector itself is about the size of a grocery bag, and contains 10 gallons of pure argon that has been liquefied by cooling it to minus 186 degrees Celsius (minus 303 degrees Fahrenheit).

The active part of the detector, swathed in Teflon, holds 50 kilograms (about 110 pounds) of active argon—hence the name DarkSide-50. At the top and bottom of the vessel are rows of photodetectors that spot the light from the collisions. In addition, copper coils collect electrons stripped from argon atoms by their recoiling sibling—this helps in determining where within the detector the collision occurred.

The argon-filled vessel sits inside a room-sized steel sphere that is suspended on stilts and filled with 7,000 gallons of a fluid called scintillator. The sphere sits inside a three-story-high cylindrical tank filled with 250,000 gallons of ultrapure water.

Both of the outer chambers will help distinguish WIMPs from cosmic-ray muons and particles called neutrons, which are emitted from trace amounts of radioactivity in the materials used to construct the detector.

A WIMP interacting with the argon will be seen nowhere else, whereas the neutron and muon will interact with both the argon and either the scintillator or water, allowing the scientists to distinguish WIMPs from the other particles.

After completing the assembly in late summer, the researchers and engineers began filling the detection chambers, first filling the inner vessel with argon, then filling the sphere and then the tank. This process took weeks. Each tank had to be checked out to make sure it was working before the next could be filled, said Shawn Westerdale, a graduate student in physics on the project.

Throughout the fall, the team met daily to discuss the progress, with some members calling in or videoconferencing from Italy as they conducted the final equipment checks.

Once the system was ready, it was time to turn it on.

"The first time you turn on a detector is the most exciting time in the life of a physicist—it is like Christmas morning," said DarkSide-50 collaborator Maria Elena Monzani of the SLAC National Accelerator Laboratory in California.

When not working in the subterranean lab, the researchers stay in the small town of Assergi, home to the above-ground facilities for Gran Sasso Lab.

Welcome to the DarkSide: Project aims to find particles of dark matter
The Darkside-50 experiment consists of three chambers. An argon-filled tank is suspended inside a liquid-filled, room-sized steel sphere, which is suspended in a three-story tank filled with ultrapure water. Researchers are looking for collisions of dark matter and visible matter in the inner chamber, and the outer chambers help distinguish dark matter particles from other particles. Credit: DarkSide-50, Gran Sasso National Laboratory

Sophomore Cynthia Steinhardt spent the summer in Assergi, helping to install parts of the detector and building software simulations to ensure that the photodetectors were working properly. During the installation, she and the others worked in class-100 clean rooms—designed to never allow more than 100 particles of 0.5 microns or larger per cubic foot of air—wearing full-body suits to protect the equipment from the small amounts of naturally occurring radioactivity in the environment.

"It was a privilege to be a part of something so important," Steinhardt said. "I was able to be involved in just about every aspect of the experiment, from coding to building and wiring, with the occasional cleaning."

Senior Maria Okounkova used the skills gained during her undergraduate education as a physics major.

"I love to code and work with numbers, so I applied my knowledge of electromagnetism and particle physics to simulations of WIMP-argon collisions," she said. "It was very rewarding to apply what I've learned at Princeton to the project."

Scaling up

The researchers began collecting data on collisions in November, but it will take some time before they are ready to publish any results. Demonstrating that they have achieved the desired level of sensitivity will be an important finding even if WIMPs are not detected, said Galbiati.

The investigators plan to increase the sensitivity this summer when they swap out the current batch of argon, which was collected from the air, with argon from a mine in Colorado. The underground argon contains 150-times fewer naturally occurring radioactive isotopes, so using it will reduce the "background noise" even further.

DarkSide-50 was supported by the National Science Foundation, the U.S. Department of Energy's Office of Science, and the Italian Institute for Nuclear Physics. The project will run for three to five years, and the researchers are already planning to enlarge DarkSide, which will increase the likelihood of detecting WIMPs. The larger detector would contain three tons of liquid argon rather than the 50 kilograms now being used.

"The detector that is the size of a grocery bag would be the size of a Chevy Suburban," Meyers said.

Between DarkSide-50 and the roughly three dozen other detectors now in operation or planned, many physicists think that dark matter particles will be found within the next five to 10 years. However, multiple experiments may be needed to confirm the sighting. A different at Gran Sasso, called DAMA, has been reporting dark matter particles since 1998, although the physics community has remained skeptical. The Large Hadron Collider, currently offline for maintenance, will begin smashing protons again in 2015 and could create particles of dark matter.

"If DarkSide-50 finds dark matter, then we will have confirmed that it is made of , and it becomes something that we can study in a laboratory," Meyers said. "Since we can only detect about three particles a year, we won't be bottling it any time soon. But because we will know how to see it, we can start to study it."

"Whatever is, it is something new, something that has never been detected before," said Taylor, who is now applying to graduate schools and hopes to continue working on the search. "That is just very exciting."

Explore further: Scientists crank up the voltage, create better dark-matter search

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billpress11
4 / 5 (1) Jan 17, 2014
I wish them luck but doubt they will succeed because dark matter is probably fleeting in and out of existence constantly and also because it is probably as small as a single wave of EMR.
Whydening Gyre
4 / 5 (1) Jan 17, 2014
Best part of it is - they got to spend a whole summer in Europe!
AmritSorli
1 / 5 (1) Jan 18, 2014
Dark matter is energy of quantum vacuum, of universal space itself.
There is no special "particle" that build dark matter.
This particle is pure math model as it is "graviton", "Higgs boson" and "gravitational waves".
Higgs boson is not more than a flux of energy of quantum vacuum caused by collisions of particles.
There is also no such a field as "Higgs field". Mass has origin in diminished energy density of quantum vacuum.
So this particle which should build dark matter will be never found.......or maybe yes, becasuse is you search for something for too long you will find it even if it does not exist. Higgs boson is a nice example of such a discovery.
Nestle
not rated yet Jan 18, 2014
Try to imagine the sphere floating at the surface of water, which is undulating both at the surface (surface waves), both beneath it (underwater longitudinal waves). The field is all about balance of surface and underwater waves. The surface waves are shielded around sphere and this is lead to the analogy of Cassimir force (result of surface waves missing at the proximity of sphere). But underwater is full of sound waves too, these waves are much faster than surface waves, but they're getting shielded too and the result is corresponding to gravity field (missing longitudinal waves, excess of virtual photons). But when the sphere is surrounded with some others, these objects shield the underwater waves around it and the result is the excess of longitudinal waves around sphere at the connection line of sphere and its neighbor(s). This excess is what the dark matter basically is.
Nestle
not rated yet Jan 18, 2014
Another analogy of both fields we can find with shore waves slowed down around island. The surface waves are slowed down into surf waves at the proximity of the coast, the underwater tsunamis are concentrated instead and they do manifest with underwater currents and increased concentration of whirlpools at the larger distance from the coast.

The underwater waves are faster than surface waves and they do manifest only with irregular noise at the water surface. When their intensity gets high, it may result into vortices. The dark matter is therefore a mixture of longitudinal - scalar waves and some vortices of vacuum - everything from Brownian noise (analogy of CMBR noise in vacuum) to real stable vortices like the Falaco solitons (analogy of neutrinos). It's quite rich mixture of various weakly interacting artifacts of different types and it can be produced in lab, because the Tesla scalar waves belong there too.
Nestle
not rated yet Jan 18, 2014
We already have both observational, both experimental evidence for this model. The shielding model of dark matter is supported with fiber shape of dark matter between galaxies and with Allais effect during solar eclipses and planetary conjunctions. The full Moon effects may belong there too. The scalar waves are produced whenever the electromagnetic field is switching on and off, not just alternate. They're interacting strongly with Dirac fermions within superconductors (and possibly graphene and topological insulators too) and they can be generated with electric impulses introduced to these materials (check the E.Podkletnov and C. Poher experiments). The problem is, the contemporary physics is focused to transverse wave models and the longitudinal waves effects are too fuzzy and indeterministic for it. But it's essentially whole half of physics missing. The only exception is the SUSY, based on duality of transverse and longitudinal torsion fields in vacuum.

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