
The helicity, or handedness, of neutrinos has only been observed in two states, left-handed neutrinos and right-handed antineutrinos. Whether these are really the only two neutrino handedness states depends on whether neutrinos are their own antiparticles.
"The best way to learn whether neutrinos are their own antiparticles would be to observe a certain kind of radioactive decay, called neutrinoless double-beta decay. It has never been detected conclusively, and if it occurs at all, it’s exceedingly rare," says Alan Poon of the Nuclear Science Division at the U.S. Department of Energy’s Lawrence Berkeley National Laboratory (Berkeley Lab).
Poon is the current executive-committee chair of the MAJORANA Collaboration, which is comprised of more than 100 researchers from 19 institutions in the United States, Canada, Russia, and Japan, and whose efforts are focused on the experiment now under construction at the Davis Campus of the Sanford Underground Research Facility (SURF) in Lead, South Dakota.
Beta decay, single and double
Ordinary beta decay is a common kind of radioactivity: an atomic nucleus changes into a different kind of element, a neighbor on the periodic table with lower mass, by emitting a beta particle - an electron or positron - plus a neutrino or an antineutrino. For example, carbon-14 transforms to nitrogen-14 when one of its neutrons turns into a proton, emitting an electron and an antineutrino. It was beta decay that led to the proposal that there must be a particle like the neutrino, since an electron alone could not account for all the energy lost in the decay.
"Double-beta decay is also possible and has been observed in a dozen different isotopes since 1986," says Poon. "But it happens at a really low rate, and not too many nuclei can do it."
The only conclusive double-beta decays seen so far involve two neutrons that change into two protons while emitting two electrons and two antineutrinos. It’s an uncommon situation, in which single beta decay is blocked because the decaying isotope’s immediate neighbor has a nucleus that’s too heavy, but the nucleus of the neighbor two places away on the periodic table does have lower mass - even though its atomic number is two places higher. Getting there requires double-beta decay.
One of the relatively few nuclei that can transform by double-beta decay is germanium-76 (76Ge), an isotope that accounts for less than eight percent of naturally occurring germanium. Germanium-76 can’t change to its neighbor, arsenic-76, but it can change to selenium-76, two places higher on the periodic table.
Many reference works refer to germanium-76 as stable, but double-beta decays of 76Ge have been observed since the 1990s, and its half-life has recently been estimated at 1.3 x 1021 years, or roughly one and a third sextillion years. That’s 100 trillion times the age of the universe. Not quite stable.
How do you detect such a rare event? If you watch a single germanium-76 atom for one and a third sextillion years, the chances are 50-50 you’ll see it decay. On the other hand, if you watch one and a third sextillion germanium-76 atoms for just one year, the chances are 50-50 that you’ll catch at least one of them decaying.
In essence, that’s what MAJORANA proposes to do. The full MAJORANA concept calls for a metric ton or so of germanium diode detectors, enriched to 86 percent 76Ge. Over the course of a year, a detector that size has a good chance of catching double-beta decays, although most will be accompanied by a pair of antineutrinos.
Searching for an absence of neutrinos
Identifying neutrinoless double-beta decays depends crucially on getting rid of background from cosmic rays and natural radioactivity in the surroundings. That’s the purpose of the MAJORANA DEMONSTRATOR: to show that achieving a low enough background is indeed possible. A mile of rock overhead is an effective shield against most cosmic ray debris, but radioactivity from the environment, including from impurities in the experiment’s own components, is harder to avoid.
Jason Detwiler of the Nuclear Science Division, who has been involved with the MAJORANA project since 2005, says, "We’re spending a lot of time modeling every one of the DEMONSTRATOR’s thousands of individual parts, to make sure we can achieve the lowest backgrounds of any experiment of this kind ever - a hundred times lower."
The MAJORANA DEMONSTRATOR will be shielded with multiple layers of copper and lead against radioactive elements in the surrounding rock, and the detector will be built from ultrapure materials. Copper components are being formed underground in special facilities at SURF, to remove natural radioactivity and prevent contamination from cosmic rays.
Equally important is the detector’s ability to distinguish the background from double-beta decays inside the detector itself. Pure germanium is ideal for this purpose, both as a source of double-beta decays and, says Detwiler, as a detector that "can register the signal of nuclear decays cleanly, beautifully, and in high resolution."
Nuclear decays and other events create charge carriers that drift toward the collecting electrode on the surface of the germanium diode. The way the carriers drift - their "pulse shape" - will clearly distinguish background events from a neutrinoless double-beta decay.







» Share this page: