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  2. Positron emission - Wikipedia

    en.wikipedia.org/wiki/Positron_emission

    Positron emission, beta plus decay, or β + decay is a subtype of radioactive decay called beta decay, in which a proton inside a radionuclide nucleus is converted into a neutron while releasing a positron and an electron neutrino (ν e). [1] Positron emission is mediated by the weak force.

  3. Double beta decay - Wikipedia

    en.wikipedia.org/wiki/Double_beta_decay

    In theory, quadruple beta decay may be experimentally observable in three of these nuclei – 96 Zr, 136 Xe, and 150 Nd – with the most promising candidate being 150 Nd. Triple beta-minus decay is also possible for 48 Ca, 96 Zr, and 150 Nd; [37] triple beta-plus decay or electron capture is also possible for 148 Gd and 154 Dy.

  4. Beta decay - Wikipedia

    en.wikipedia.org/wiki/Beta_decay

    The two types of beta decay are known as beta minus and beta plus.In beta minus (β −) decay, a neutron is converted to a proton, and the process creates an electron and an electron antineutrino; while in beta plus (β +) decay, a proton is converted to a neutron and the process creates a positron and an electron neutrino. β + decay is also known as positron emission.

  5. Neutrinoless double beta decay - Wikipedia

    en.wikipedia.org/wiki/Neutrinoless_double_beta_decay

    Neutrinoless double beta decay can only occur if the neutrino particle is Majorana, [11] and; there exists a right-handed component of the weak leptonic current or the neutrino can change its handedness between emission and absorption (between the two W vertices), which is possible for a non-zero neutrino mass (for at least one of the neutrino ...

  6. Beta particle - Wikipedia

    en.wikipedia.org/wiki/Beta_particle

    A beta particle, also called beta ray or beta radiation (symbol β), is a high-energy, high-speed electron or positron emitted by the radioactive decay of an atomic nucleus, known as beta decay. There are two forms of beta decay, β − decay and β + decay, which produce electrons and positrons, respectively. [2] Beta particles with an energy ...

  7. Enriched Xenon Observatory - Wikipedia

    en.wikipedia.org/wiki/Enriched_Xenon_Observatory

    In August 2011, EXO-200 was the first experiment to observe double beta decay of 136 Xe, with a half life of 2.11×10 21 years. [5] This is the slowest directly observed process. An improved half life of 2.165 ±0.016(stat) ±0.059(sys) × 10 21 years was published in 2014. [6] EXO set a limit on neutrinoless beta decay of 1.6×10 25 years in ...

  8. Decay energy - Wikipedia

    en.wikipedia.org/wiki/Decay_energy

    The decay energy is the mass difference Δm between the parent and the daughter atom and particles. It is equal to the energy of radiation E . If A is the radioactive activity , i.e. the number of transforming atoms per time, M the molar mass, then the radiation power P is:

  9. Valley of stability - Wikipedia

    en.wikipedia.org/wiki/Valley_of_stability

    The difference between the initial and final nuclide binding energies is carried away by the kinetic energies of the decay products, often the beta particle and its associated neutrino. [3] The concept of the valley of stability is a way of organizing all of the nuclides according to binding energy as a function of neutron and proton numbers. [1]