Stalking the Neutrinoless Double Beta Decay

Stalking the Neutrinoless Double Beta Decay
Conceptual drawing of the germanium-76 detector array.
(PhysOrg.com) -- The hunt for the elusive neutrino mass has officially begun. This difficult-to-detect elementary particle travels close to the speed of light, is electrically neutral, and can pass through ordinary matter almost undisturbed.

In FY 2010 DOE’s Office of Nuclear Physicsallocated $20 million over the next four years to the Majorana Demonstrator Project, which is aimed at capturing neutrinoless double beta decay events. “If we are able to measure the rate of neutrinoless double decay, we can infer the absolute mass of the neutrino,” said deputy project manager, Dick Kouzes.

Kouzes, a nuclear scientist who has studied this question since the 1980s, says the discovery would lead to a revision of the Standard Model of particle physics that governs the laws of all in the universe, essentially redefining the laws of physics.

Developed in the 1930s, the original theory that hypothesized the neutrino assumed it had no mass. Later, researchers found neutrinos have three different states, or what the researchers coined as “three flavors.” Experiments to measure solar, cosmic and accelerator-produced showed that the neutrino oscillates between these states. Only a particle with a mass could show these flavor oscillations.

But, to date, the neutrino’s mass has not been measured.

In addition to Kouzes, PNNL scientists James Fast, Eric Hoppe, John Orrell, Craig Aalseth, Erin Fuller, Harry Miley, James Ely, Todd Hossbach, Jeremy Kephart and Martin Keillor are part of the 100-strong collaboration managed by Oak Ridge National Laboratory. PNNL originally designed the experiment and developed the ultra-low background detection capabilities slated to be used in it.

Stalking the Neutrinoless Double Beta Decay
Section view of a germanium detector showing its electrical potential. The point contact is on the bottom and the electrical potential drops off to the outer wall of the cylinder.

The know-how came from our historical strength in detecting signatures of the production, movement and trafficking of weapons of destruction,” said Kouzes. In addition to helping with project management, PNNL is responsible for designing the detector assembly, producing the highly purified copper needed for the detector assembly, and ensuring the detector assembly meets the background requirements.

With the help of a 60-kilogram array of ultrapure germanium-76 detectors housed deep underground where external background sources are at a minimum, the collaborators hope to observe the handful of neutrinoless double beta decay events taking place each year. They will be looking for a characteristic spectrum to emerge from the detectors when a neutrinoless double beta decay is detected - “like a rounded curve with a bump at the end on top of background noise” is how Kouzes put it. The detector is slated to be in place, almost a mile underground, by 2012.

The Majorana Demonstrator Project is high risk discovery science. If the first experiment is fruitful, the team plans to upgrade to a one metric ton germanium-76 detector array within 5 years.


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Citation: Stalking the Neutrinoless Double Beta Decay (2010, February 12) retrieved 25 June 2019 from https://phys.org/news/2010-02-stalking-neutrinoless-beta.html
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Feb 12, 2010
EXCITING IMO, given the origin of the dark/light matter balance hypothesis. i.e. neutron decay & neutrino annihilation

Feb 12, 2010
There is an apparent similarity in experimental arrangement during finding of neutrinoless double beta decay and WIMPS forming dark matter. Maybe Majorana neutrino is in fact product of neutrino-anti-neutrino coupling by Higgs field in analogy to Yukawa coupling of top–antitop quark pairs observed already at Tevatron.

It would be a nice demonstration of AdS/CFT correspondence between physics of lowest and highest energy density observable in accordance to "Mobius strip" topology of Universe.

http://www.physor...561.html

Feb 13, 2010
http://en.wikiped...Neutrino

See mass section for eigenstates etc.

Wiki-disclaimer: Your mileage may vary.

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