enow.com Web Search

Search results

  1. Results from the WOW.Com Content Network
  2. Carbon-14 - Wikipedia

    en.wikipedia.org/wiki/Carbon-14

    Carbon-14 undergoes beta decay: . 14 6 C → 14 7 N + e − + ν e + 0.156.5 MeV. By emitting an electron and an electron antineutrino, one of the neutrons in carbon-14 decays to a proton and the carbon-14 (half-life of 5700 ± 30 years [1]) decays into the stable (non-radioactive) isotope nitrogen-14.

  3. 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.

  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. Radioactive decay - Wikipedia

    en.wikipedia.org/wiki/Radioactive_decay

    Carbon-14 has a half-life of 5700(30) years [27] and a decay rate of 14 disintegrations per minute (dpm) per gram of natural carbon. If an artifact is found to have radioactivity of 4 dpm per gram of its present C, we can find the approximate age of the object using the above equation:

  6. Valley of stability - Wikipedia

    en.wikipedia.org/wiki/Valley_of_stability

    A common example of an unstable nuclide is carbon-14 that decays by beta decay 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 and a beta particle and an electron antineutrino are emitted.

  7. Weak interaction - Wikipedia

    en.wikipedia.org/wiki/Weak_interaction

    Most fermions decay by a weak interaction over time. Such decay makes radiocarbon dating possible, as carbon-14 decays through the weak interaction to nitrogen-14. It can also create radioluminescence, commonly used in tritium luminescence, and in the related field of betavoltaics [4] (but not similar to radium luminescence).

  8. Common beta emitters - Wikipedia

    en.wikipedia.org/wiki/Common_beta_emitters

    Tritium is a low-energy beta emitter commonly used as a radiotracer in research and in traser [check spelling] self-powered lightings.The half-life of tritium is 12.3 years. The electrons from beta emission from tritium are so low in energy (average decay energy 5.7 keV) that a Geiger counter cannot be used to detect the

  9. 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.