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The neutrinoless double beta decay (0νββ) is a commonly proposed and experimentally pursued theoretical radioactive decay process that would prove a Majorana nature of the neutrino particle. To this day, it has not been found.
The discovery of the neutrinoless double beta decay could shed light on the absolute neutrino masses and on their mass hierarchy (Neutrino mass). It would mean the first ever signal of the violation of total lepton number conservation. A Majorana nature of neutrinos would confirm that the neutrino's own antiparticle is no different than itself, i.e. it is its own antiparticle.
To search for neutrinoless double beta decay, there are currently a number of experiments underway, with several future experiments for increased sensitivity proposed as well.
Back in 1939, Wendell H. Furry proposed the idea of the Majorana nature of the neutrino, which was associated with beta decays. Furry stated the transition probability to even be higher for the neutrinoless double beta decay. It was the first idea proposed to search for the violation of lepton number conservation. It has, since then, drawn attention to it for being useful to study the nature of neutrinos (see quote).
[T]he 0ν mode [...] which violates the lepton number and has been recognized since a long time as a powerful tool to test neutrino properties.
— Oliviero Cremonesi
The Italian physicist Ettore Majorana first introduced the concept of a particle being its own antiparticle. Particles' nature was subsequently named after him as Majorana particles. The neutrinoless double beta decay is one method to search for the possible Majorana nature of neutrinos.
Neutrinos are conventionally produced in weak decays. Weak beta decays normally produce one electron (or positron), emit an antineutrino (or neutrino) and increase the nucleus' proton number by one. The nucleus' mass (i.e. binding energy) is then lower and thus more favorable. There exists a number of elements that can decay into a nucleus of lower mass, but they cannot emit one electron only because the resulting nucleus is kinematically (that is, in terms of energy) not favorable (its energy would be higher). These nuclei can only decay by emitting two electrons (that is, via double beta decay). There is about a dozen confirmed cases of nuclei that can only decay via double beta decay. The corresponding decay equation is:
It is a weak process of second order. A simultaneous decay of two nucleons in the same nucleus is extremely unlikely. Thus, the experimentally observed lifetimes of such decay processes are in the range of years. A number of isotopes have been observed already to show this two-neutrino double beta decay.
This conventional double beta decay is allowed in the Standard Model of particle physics. It has thus both a theoretical and an experimental foundation.
If the nature of the neutrinos is Majorana, then they can be emitted and absorbed in the same process without showing up in the corresponding final state. As Dirac particles, both the neutrinos produced by the decay of the W bosons would be emitted, and not absorbed after.
The neutrinoless double beta decay can only occur if
The simplest decay process is known as the light neutrino exchange. It features one neutrino emitted by one nucleon and absorbed by another nucleon (see figure to the right). In the final state, the only remaining parts are the nucleus (with its changed proton number ) and two electrons:
The two electrons are emitted quasi-simultaneously.
The two resulting electrons are then the only emitted particles in the final state and must carry approximately the difference of the sums of the binding energies of the two nuclei before and after the process as their kinetic energy. The heavy nuclei do not carry significant kinetic energy. The electrons will be emitted back-to-back due to momentum conservation.
In that case, the decay rate can be calculated with
where denotes the phase space factor, the (squared) matrix element of this nuclear decay process (according to the Feynman diagram), and the square of the effective Majorana mass.
First, the effective Majorana mass can be obtained by
where are the Majorana neutrino masses (three neutrinos ) and the elements of the neutrino mixing matrix (see PMNS matrix). Contemporary experiments to find neutrinoless double beta decays (see section on experiments) aim at both the proof of the Majorana nature of neutrinos and the measurement of this effective Majorana mass (can only be done if the decay is actually generated by the neutrino masses).
The nuclear matrix element (NME) cannot be measured independently;[why?] it must, but also can, be calculated. The calculation itself relies on sophisticated nuclear many-body theories and there exist different methods to do this. The NME differs also from nucleus to nucleus (i.e. chemical element to chemical element). Today, the calculation of the NME is a significant problem and it has been treated by different authors in different ways. One question is whether to treat the range of obtained values for as the theoretical uncertainty and whether this is then to be understood as a statistical uncertainty. Different approaches are being chosen here. The obtained values for often vary by factors of 2 up to about 5. Typical values lie in the range of from about 0.9 to 14, depending on the decaying nucleus/element.
Lastly, the phase-space factor must also be calculated. It depends on the total released kinetic energy (, i.e. "-value") and the atomic number . Methods utilize Dirac wave functions, finite nuclear sizes and electron screening. There exist high-precision results for for various nuclei, ranging from about 0.23 (for ), and 0.90 () to about 24.14 ().
It is believed that, if neutrinoless double beta decay is found under certain conditions (decay rate compatible with predictions based on experimental knowledge about neutrino masses and mixing), this would indeed "likely" point at Majorana neutrinos as the main mediator (and not other sources of new physics). There are 35 nuclei that can undergo neutrinoless double beta decay (according to the aforementioned decay conditions).
Nine different candidates of nuclei are being considered in experiments to confirm neutrinoless double beta-decay: . They all have arguments for and against their use in an experiment. Factors to be included and revised are natural abundance, reasonably priced enrichment, and a well understood and controlled experimental technique. The higher the -value, the better are the chances of a discovery, in principal. The phase-space factor , and thus the decay rate, grows with .
Experimentally of interest and thus measured is the sum of the kinetic energies of the two emitted electrons. It should equal the -value of the respective nucleus for neutrinoless double beta emission.
The table shows a summary of the currently best limits on the lifetime of 0νββ. From this, it can be deduced that neutrinoless double beta decay is an extremely rare process - if it occurs at all.
The so-called "Heidelberg-Moscow collaboration" (HDM) of the German Max-Planck-Institut für Kernphysik and the Russian science center Kurchatov Institute in Moscow famously claimed to have found "evidence for neutrinoless double beta decay". Initially, in 2001 the collaboration announced a 2.2σ, or a 3.1σ (depending on the used calculation method) evidence. The decay rate was found to be around years. This result has been topic of discussions between many scientists and authors. To this day, no other experiment has ever confirmed or approved the result of the HDM group. Instead, recent results from the GERDA experiment for the lifetime limit clearly disfavor and reject the values of the HDM collaboration.
Neutrinoless double beta decay has not yet been found.