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  2. Radioactive decay - Wikipedia

    en.wikipedia.org/wiki/Radioactive_decay

    v. t. e. Radioactive decay (also known as nuclear decay, radioactivity, radioactive disintegration, or nuclear disintegration) is the process by which an unstable atomic nucleus loses energy by radiation. A material containing unstable nuclei is considered radioactive. Three of the most common types of decay are alpha, beta, and gamma decay.

  3. Astatine - Wikipedia

    en.wikipedia.org/wiki/Astatine

    Astatine-210 and most of the lighter isotopes exhibit beta plus decay (positron emission), astatine-217 and heavier isotopes except astatine-218 exhibit beta minus decay, while astatine-211 undergoes electron capture. [5] The most stable isotope is astatine-210, which has a half-life of 8.1 hours.

  4. Radiocarbon dating - Wikipedia

    en.wikipedia.org/wiki/Radiocarbon_dating

    C in a sample was to detect the radioactive decay of individual carbon atoms. [59] In this approach, what is measured is the activity, in number of decay events per unit mass per time period, of the sample. [60] This method is also known as "beta counting", because it is the beta particles emitted by the decaying 14 C atoms that are detected. [63]

  5. Actinide - Wikipedia

    en.wikipedia.org/wiki/Actinide

    The beta-minus decay, marked with an arrow pointing up-left, plays a major role for the balance of the particle densities of the nuclides. Nuclides decaying by positron emission (beta-plus decay) or electron capture (ϵ) do not occur in a nuclear reactor except as products of knockout reactions; their decays are marked with arrows pointing down ...

  6. Neutron - Wikipedia

    en.wikipedia.org/wiki/Neutron

    These reactions are a form of radioactive decay known as beta decay. [16] Beta decay, in which neutrons decay to protons, or vice versa, is governed by the weak force, and it requires the emission or absorption of electrons and neutrinos, or their antiparticles. [17] The neutron and proton decay reactions are: n 0 → p + + e − + ν e. where ...

  7. Supernova - Wikipedia

    en.wikipedia.org/wiki/Supernova

    56 Ni is radioactive and decays into 56 Co by beta plus decay (with a half life of six days) and gamma rays. 56 Co itself decays by the beta plus path with a half life of 77 days into stable 56 Fe. These two processes are responsible for the electromagnetic radiation from type Ia supernovae.

  8. Americium - Wikipedia

    en.wikipedia.org/wiki/Americium

    Nearly all (99.541%) of 242m1 Am decays by internal conversion to 242 Am and the remaining 0.459% by α-decay to 238 Np. The latter subsequently decays to 238 Pu and then to 234 U. [14] Americium-243 transforms by α-emission into 239 Np, which converts by β-decay to 239 Pu, and the 239 Pu changes into 235 U by emitting an α-particle.

  9. Hydrogen isotope biogeochemistry - Wikipedia

    en.wikipedia.org/wiki/Hydrogen_isotope...

    Hydrogen isotope biogeochemistry. Hydrogen isotope biogeochemistry (HIBGC) is the scientific study of biological, geological, and chemical processes in the environment using the distribution and relative abundance of hydrogen isotopes. Hydrogen has two stable isotopes, protium 1 H and deuterium 2 H, which vary in relative abundance on the order ...