Double beta decay

Double beta decay is a radioactive decay process where a nucleus releases two beta rays as a single process.

In double-beta decay, two neutrons in the nucleus are converted to protons, and two electrons and two electron antineutrinos are emitted. In the process of beta minus decay, unstable nuclei decay by converting a neutron in the nucleus to a proton and emitting an electron and an electron antineutrino. In order for 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 nucleus with atomic number one higher has a smaller binding energy, preventing beta decay from occurring. However, the nucleus with atomic number two higher, selenium-76, has a larger binding energy, so the double-beta decay process is allowed.

Although efforts to observe the process date back to 1948, it wasn't observed in a laboratory setting until 1986. Geochemical observation of the decay products (by extraction of Kr and Xe from very old Se and Te minerals) are known since 1950. Double-beta decay is the rarest known kind of radioactive decay; it has been observed for only 10 isotopes, and all of them have a mean life time of more than 10¹⁹ yr.

For some nuclei, the process occurs as conversion of two protons to neutrons, with emission of two electron neutrinos and absorption of 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 branch is accessible, with capture of one orbital electron and emission of one positron. When the mass difference is more than 2.044 MeV/c² (four electron masses), the emission of two positrons is possible. These theoretically possible double-beta decay branches have not yet been observed.

List of known double-beta decay isotopes

More than 60 naturally occurring isotopes are capable of undergoing double-beta decay. Only ten of them were observed to decay via the two-neutrino mode:

, , ,, , , , , , and .

Many isotopes are, in theory, capable both of double-beta decay and other decays. In most cases, the double-beta decay is so rare as to be nearly impossible to observe against the background of other radiation. However, the double-beta decay rate of (also an alpha emitter) has been measured radiochemically; is produced by this type of radioactivity. Two of the nuclides ( and ) from the list above can decay also via single beta decay but this decay is extremely suppressed and has never been observed.

Neutrinoless double-beta decay

of neutrinoless double-beta decay, with two neutrons decaying to two protons. The only emitted products in this process are two electrons, which can only occur if the neutrino and antineutrino are the same particle (i.e. Majorana neutrinos) so the same neutrino can be emitted and absorbed within the nucleus. In conventional double-beta decay, two antineutrinos - one arising from each W vertex - are emitted from the nucleus, in addition to the two electrons. The detection of neutrinoless double-beta decay is thus a sensitive test of whether neutrinos are Majorana particles.]]

The processes described in the previous section are also known as two neutrino double-beta decay, as two neutrinos (or antineutrinos) are emitted. If the neutrino is a Majorana particle (meaning that 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. In the simplest theoretical treatment of neutrinoless double-beta decay (light neutrino exchange), in essence the two neutrinos annihilate each other, or equivalently, one nucleon absorbs the neutrino emitted by another nucleon of the nucleus.

The neutrinos in the above diagram are virtual particles. With only the two electrons in the final state, the total kinetic energy of the two electrons would be approximately the difference in binding energy between the initial and final state nuclei (with the recoil of the nucleus accounting for the rest of the available energy). To a very good approximation, the two electrons are emitted back-to-back to conserve momentum.

The decay rate for this process is given (approximately) by

:$\backslash Gamma\; =\; ~~~~\{G\; |M|^2\; |m\_\{\backslash beta\; \backslash beta\}|^2\},$

where $G$ is the two-body phase-space factor, $M$ is the nuclear matrix element, and m_ββ is the so called effective Majorana neutrino mass given by

:$m\_\{\backslash beta\; \backslash beta\}\; =\; \backslash sum\_\{i=1\}^3\; m\_i\; U^2\_\{ei\}.$

In this latter expression, the m_i are the neutrino masses (of the i^th mass eigenstate), and the U_ei are elements of the Pontecorvo–Maki–Nakagawa–Sakata (PMNS) matrix. Hence the observation of neutrinoless double-beta decay, in addition to confirming the Majorana nature of the neutrino, would give information on the absolute neutrino mass scale, and potentially also on the neutrino mass hierarchy and the Majorana phases appearing in the PMNS matrix.

Neutrinoless double-beta decay experiments

Numerous experiments have been carried out to search for neutrinoless double-beta decay. Some recent and proposed future experiments include:

Completed experiments:

* Gotthard TPC

* Heidelberg-Moscow

* IGEX

* NEMO1 and 2

Current and proposed experiments

* COBRA

* CUORICINO and CUORE

* EXO

* GERDA

* MAJORANA

* MOON

* NEMO-3 and SuperNEMO

* SNO+

Klapdor-Kleingrothaus et al.'s claimed observation of neutrinoless double-beta decay

A subgroup of the Heidelberg-Moscow collaboration led by H. V. Klapdor-Kleingrothaus published a series of controversial papers claiming to have observed neutrinoless double-beta decay in with statistical significance of > 99.9999998%. This claim has been criticized by many in the nuclear and particle physics communities, but Klapdor-Kleingrothaus et al. have vigorously defended their work. Their measured value of m_ββ between ~0.2-0.5 eV (depending on the choice of nuclear matrix element) has yet to be confirmed by other experiments.

The following lists, in chronological order, the key publications and preprints related to the claim and the criticism thereof.

16 (2001) p. 2409,">H. V. Klapdor-Kleingrothaus et al., "Evidence for Neutrinoless Double Beta Decay", Mod. Phys. Lett. A 16 (2001) p. 2409, arXiv:hep-ph/0201231. This is the original paper, claiming a 2-3σ observation (depending on the statistical method used to measure the significance).

17 (2002) p. 1475,">C. E. Aalseth et al., "Comment on 'Evidence for Neutrinoless Double Beta Decay'", Mod. Phys. Lett. A 17 (2002) p. 1475, arXiv:hep-ex/0202018.

H. V. Klapdor-Kleingrothaus, "Reply to a Comment of article 'Evidence for Neutrinoless Double Beta Decay'", arXiv:hep-ph/0205228 (2002) (not peer-reviewed).

H. L. Harney, "Reply to the Comment on 'Evidence for Neutrinoless Double Beta Decay'", arXiv:hep-ph/0205293 (2002) (not peer-reviewed).

32 (2002) 1181,">H. V. Klapdor-Kleingrothaus et al., "Neutrinoless Double Beta Decay: Status of Evidence", Found. Phys. 32 (2002) 1181, arXiv:hep-ph/0302248.

76Ge in Gran Sasso 1990–2003", Phys. Lett. B 586 (2004) p. 198.">H. V. Klapdor-Kleingrothaus et al., "Search for neutrinoless double beta decay with enriched ⁷⁶Ge in Gran Sasso 1990–2003", Phys. Lett. B 586 (2004) p. 198. Statistical significance increases to >4σ.

21 (2006) p. 1547.">H. V. Klapdor-Kleingrothaus and I. V. Krivosheina, "The Evidence for the Observation of 0νββ Decay: the Identification of 0νββ Events from the Full Spectra", Mod. Phys. Lett. A 21 (2006) p. 1547. Statistical significance increases to >6σ.

See also

Double electron capture

Beta decay

Neutrino

Particle radiation

Radioactive isotope

References

Double beta decay on arxiv.org

Category:Nuclear physics Category:Radioactivity Category:Particle physics