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  2. Beta decay - Wikipedia

    en.wikipedia.org/wiki/Beta_decay

    An example of electron emission (β − decay) is the decay of carbon-14 into nitrogen-14 with a half-life of about 5,730 years: 14 6 C → 14 7 N + e − + ν e. In this form of decay, the original element becomes a new chemical element in a process known as nuclear transmutation.

  3. List of nuclides - Wikipedia

    en.wikipedia.org/wiki/List_of_nuclides

    The next group is the primordial radioactive nuclides. These have been measured to be radioactive, or decay products have been identified in natural samples (tellurium-128, barium-130). There are 35 of these (see these nuclides), of which 25 have half-lives longer than 10 13 years. With most of these 25, decay is difficult to observe and for ...

  4. List of radioactive nuclides by half-life - Wikipedia

    en.wikipedia.org/wiki/List_of_radioactive...

    This is a list of radioactive nuclides (sometimes also called isotopes), ordered by half-life from shortest to longest, in seconds, minutes, hours, days and years. Current methods make it difficult to measure half-lives between approximately 10 −19 and 10 −10 seconds.

  5. Primordial nuclide - Wikipedia

    en.wikipedia.org/wiki/Primordial_nuclide

    For three elements (indium, tellurium, and rhenium) a very long-lived radioactive primordial nuclide is more abundant than a stable nuclide. The longest-lived radionuclide known, 128 Te, has a half-life of 2.2 × 10 24 years: 1.6 × 10 14 times the age of the Universe. Only four of these 35 nuclides have half-lives shorter than, or equal to ...

  6. Neutron - Wikipedia

    en.wikipedia.org/wiki/Neutron

    A fast neutron is a free neutron with a kinetic energy level close to 1 MeV (1.6 × 10 −13 J), hence a speed of ~ 14 000 km/s (~ 5% of the speed of light). They are named fission energy or fast neutrons to distinguish them from lower-energy thermal neutrons, and high-energy neutrons produced in cosmic showers or accelerators.

  7. Carbon-13 - Wikipedia

    en.wikipedia.org/wiki/Carbon-13

    Bulk carbon-13 for commercial use, e.g. in chemical synthesis, is enriched from its natural 1% abundance. Although carbon-13 can be separated from the major carbon-12 isotope via techniques such as thermal diffusion, chemical exchange, gas diffusion, and laser and cryogenic distillation, currently only cryogenic distillation of methane (boiling point −161.5°C) or carbon monoxide (b.p. − ...

  8. Spontaneous fission - Wikipedia

    en.wikipedia.org/wiki/Spontaneous_fission

    Spontaneous fission (SF) is a form of radioactive decay in which a heavy atomic nucleus splits into two or more lighter nuclei. In contrast to induced fission, there is no inciting particle to trigger the decay; it is a purely probabilistic process.

  9. Isotopes of thorium - Wikipedia

    en.wikipedia.org/wiki/Isotopes_of_thorium

    Ionium was a name given early in the study of radioactive elements to the 230 Th isotope produced in the decay chain of 238 U before it was realized that ionium and thorium are chemically identical. The symbol Io was used for this supposed element.