Double beta decay
In nuclear physics, double beta decay is a type of radioactive decay in which two protons are simultaneously transformed into two neutrons, or vice versa, inside an atomic nucleus. As in single beta decay, this process allows the atom to move closer to the optimal ratio of protons and neutrons. As a result of this transformation, the nucleus emits two detectable beta particles, which are electrons or positrons.
There are two types of double beta decay: ordinary double beta decay and neutrinoless double beta decay. In ordinary double beta decay, which has been observed in several isotopes, two electrons and two electron antineutrinos are emitted from the decaying nucleus. In neutrinoless double beta decay, a hypothesized process that has never been observed, only electrons would be emitted.
The idea of double beta decay was first proposed by Maria Goeppert-Mayer in 1935. In 1937, Ettore Majorana demonstrated that all results of beta decay theory remain unchanged if the neutrino were its own antiparticle, now known as a Majorana particle. In 1939, Wendell H. Furry proposed that if neutrinos are Majorana particles, then double beta decay can proceed without the emission of any neutrinos, via the process now called neutrinoless double beta decay. It is not yet known whether the neutrino is a Majorana particle and, relatedly, whether neutrinoless double beta exists in nature.
In 1930–40s, parity violation in weak interactions was not known, and consequently calculations showed that neutrinoless double beta decay should be much more likely to occur than ordinary double beta decay, if neutrinos were Majorana particles. The predicted half-lives were on the order of 1015–16 years. Efforts to observe the process in laboratory date back to at least 1948 when Edward L. Fireman made the first attempt to directly measure the half-life of the 124
isotope with a geiger counter. Radiometric experiments through about 1960 produced negative results or false positives, not confirmed by later experiments. In 1950, for the first time the double beta decay half-life of 130
was measured by geochemical methods to be 1.4×1021 years, reasonably close to the modern value.
In 1956, after the V-A nature of weak interactions was established, it became clear that the half-life of neutrinoless double beta decay would significantly exceed that of ordinary double beta decay. Despite significant progress in experimental techniques in 1960–70s, double beta decay was not observed in a laboratory until the 1980s. Experiments had only been able to establish the lower bound for the half-life—about 1021 years. At the same time, geochemical experiments detected the double beta decay of 82
Double beta decay was first observed in a laboratory in 1987 by the group of Michael Moe at UC Irvine in 82
. Since then, many experiments have observed ordinary double beta decay in other isotopes. None of those experiments have produced positive results for the neutrinoless process, raising the half-life lower bound to approximately 1025 years. Geochemical experiments continued through the 1990s, producing positive results for several isotopes. Double beta decay is the rarest known kind of radioactive decay; as of 2012 it has been observed in only 13 isotopes (including double electron capture in 130
observed in 2001 and 78
observed in 2013), and all have a mean lifetime over 1018 yr (table below).
Ordinary double beta decayEdit
In a typical double beta decay, two neutrons in the nucleus are converted to protons, and two electrons and two electron antineutrinos are emitted. The process can be thought as two simultaneous beta minus decays. In order for (double) beta decay to be possible, the final nucleus must have a larger binding energy than the original nucleus. For some nuclei, such as germanium-76, the isobar one atomic number higher (arsenic-76) has a smaller binding energy, preventing single beta decay. However, the isobar with atomic number two higher, selenium-76, has a larger binding energy, so double beta decay is allowed.
where the subscripts refer to each electron, T is kinetic energy, F(Z, T) is the Fermi Function with Z the charge of the final-state nucleus, p is momentum, v is velocity in units of c, cosθ is the angle between the electrons, and Q is the Q value of the decay.
For some nuclei, the process occurs as conversion of two protons to neutrons, emitting two electron neutrinos and absorbing two orbital electrons (double electron capture). If the mass difference between the parent and daughter atoms is more than 1.022 MeV/c2 (two electron masses), another decay is accessible, capture of one orbital electron and emission of one positron. When the mass difference is more than 2.044 MeV/c2 (four electron masses), emission of two positrons is possible. These theoretical decay branches have not been observed.
Known double beta decay isotopesEdit
There are 35 naturally occurring isotopes capable of double beta decay. In practice, the decay can be observed when the single beta decay is forbidden by energy conservation. This happens for elements with an even atomic number and even neutron number, which are more stable due to spin-coupling. When single beta decay or alpha decay also occur, the double beta decay rate is generally too low to observe. However, the double beta decay of 238
(also an alpha emitter) has been measured radiochemically. Two other nuclides in which double beta decay has been observed, 48
, can also theoretically single beta decay, but this decay extremely suppressed and has never been observed.
Thirteen isotopes have been experimentally observed undergoing two-neutrino double beta decay (β–β–) or double electron capture (εε). The table below contains nuclides with the latest experimentally measured half-lives, as of December 2016. Where two errors are specified, the first one is statistical error and the second is systematic.
|Nuclide||Half-life, 1021 years||Mode||Transition||Method||Experiment|
−0.006 ± +0.012
|0.096 ± 0.003 ± 0.010||β–β–||direct||NEMO-3|
|0.0235 ± 0.0014 ± 0.0016||β–β–||direct||NEMO-3|
|0.00693 ± 0.00004||β–β–||direct||NEMO-3|
−0.08 ± 0.07
|β–β–||0+→ 0+1||Ge coincidence|
|0.028 ± 0.001 ± 0.003
|7200 ± 400
1800 ± 700
|0.82 ± 0.02 ± 0.06||β–β–||direct||CUORE-0|
|2.165 ± 0.016 ± 0.059||β–β–||direct||EXO-200|
|(0.5 – 2.7)||εε||geochemical|||
−0.00022 ± 0.00063
|β–β–||0+→ 0+1||Ge coincidence|
|2.0 ± 0.6||β–β–||radiochemical|||
Neutrinoless double beta decayEdit
If the neutrino is a Majorana particle (i.e., the antineutrino and the neutrino are actually the same particle), and at least one type of neutrino has non-zero mass (which has been established by the neutrino oscillation experiments), then it is possible for neutrinoless double beta decay to occur. Neutrinoless double beta decay is a lepton number violating process. In the simplest theoretical treatment, known as light neutrino exchange, a nucleon absorbs the neutrino emitted by another nucleon. The exchanged neutrinos are virtual particles.
With only two electrons in the final state, the electrons' total kinetic energy would be approximately the binding energy difference of the initial and final nuclei, with the nuclear recoil accounting for the rest. Because of momentum conservation, electrons are generally emitted back-to-back. The decay rate for this process is given by
where G is the two-body phase-space factor, M is the nuclear matrix element, and mββ is the effective Majorana mass of the electron neutrino. In the context of light Majorana neutrino exchange, mββ is given by
where mi are the neutrino masses and the Uei are elements of the Pontecorvo–Maki–Nakagawa–Sakata (PMNS) matrix. Therefore, observing neutrinoless double beta decay, in addition to confirming the Majorana neutrino nature, can give information on the absolute neutrino mass scale and Majorana phases in the PMNS matrix, subject to interpretation through theoretical models of the nucleus, which determine the nuclear matrix elements, and models of the decay.
Numerous experiments have searched for neutrinoless double beta decay. The best-performing experiments have a high mass of the decaying isotope and low backgrounds, with some experiments able to perform particle discrimination and electron tracking. In order to remove backgrounds from cosmic rays, most experiments are located in underground laboratories around the world.
Recent and proposed experiments include:
- Completed experiments:
- Experiments taking data as of November 2017:
- Proposed/future experiments:
- CANDLES, 48Ca in CaF2, at Kamioka Observatory
- MOON, developing 100Mo detectors
- AMoRE, 100Mo enriched CaMoO4 crystals at YangYang underground laboratory
- LUMINEU, exploring 100Mo enriched ZnMoO4 crystals at LSM, France.
- NEXT, a Xenon TPC. NEXT-DEMO ran and NEXT-100 will run in 2016.
- SNO+, a liquid scintillator, will study 130Te
- SuperNEMO, a NEMO upgrade, will study 82Se
- TIN.TIN, a 124Sn detector at INO
While some experiments have claimed a discovery of neutrinoless double beta decay, modern searches have found no evidence for the decay.
Some members of the Heidelberg-Moscow collaboration claimed a detection of neutrinoless beta decay in 76Ge in 2001. This claim was criticized by outside physicists as well as other members of the collaboration. In 2006, a refined estimate by the same authors stated the half-life was 2.3×1025 years. This half-life has been excluded at high confidence by other experiments, including in 76Ge by GERDA.
As of 2017, the strongest limits on neutrinoless double beta decay have come from GERDA in 76Ge, CUORE in 130Te, and EXO-200 and KamLAND-Zen in 136Xe.
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