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  2. Alpha particle - Wikipedia

    en.wikipedia.org/wiki/Alpha_particle

    Secondly, he found the charge-to-mass ratio of alpha particles to be half that of the hydrogen ion. Rutherford proposed three explanations: 1) an alpha particle is a hydrogen molecule (H 2) with a charge of 1 e; 2) an alpha particle is an atom of helium with a charge of 2 e; 3) an alpha particle is half a helium atom with a charge of 1 e.

  3. Alpha decay - Wikipedia

    en.wikipedia.org/wiki/Alpha_decay

    Computing the total disintegration energy given by the equation = (), where m i is the initial mass of the nucleus, m f is the mass of the nucleus after particle emission, and m p is the mass of the emitted (alpha-)particle, one finds that in certain cases it is positive and so alpha particle emission is possible, whereas other decay modes ...

  4. Radioactive decay - Wikipedia

    en.wikipedia.org/wiki/Radioactive_decay

    The alpha particle is an especially strongly bound nucleus, helping it win the competition more often. [57]: 872 However some nuclei break up or fission into larger particles and artificial nuclei decay with the emission of single protons, double protons, and other combinations. [55] Beta decay transforms a neutron into proton or vice versa.

  5. Cosmic ray spallation - Wikipedia

    en.wikipedia.org/wiki/Cosmic_ray_spallation

    An example of cosmic ray spallation is a neutron hitting a nitrogen-14 nucleus in the Earth's atmosphere, yielding a proton, an alpha particle, and a beryllium-10 nucleus, which eventually decays to boron-10. Alternatively, a proton can hit oxygen-16, yielding two protons, a neutron, and again an alpha particle and a beryllium-10 nucleus.

  6. Cosmic ray - Wikipedia

    en.wikipedia.org/wiki/Cosmic_ray

    Primary cosmic rays are composed mainly of protons and alpha particles (99%), with a small amount of heavier nuclei (≈1%) and an extremely minute proportion of positrons and antiprotons. [10] Secondary cosmic rays, caused by a decay of primary cosmic rays as they impact an atmosphere, include photons, hadrons , and leptons , such as electrons ...

  7. Photodisintegration - Wikipedia

    en.wikipedia.org/wiki/Photodisintegration

    The incoming gamma ray effectively knocks one or more neutrons, protons, or an alpha particle out of the nucleus. [1] The reactions are called (γ,n), (γ,p), and (γ,α), respectively. Photodisintegration is endothermic (energy absorbing) for atomic nuclei lighter than iron and sometimes exothermic (energy releasing) for atomic nuclei heavier ...

  8. Weak interaction - Wikipedia

    en.wikipedia.org/wiki/Weak_interaction

    boson (a particle with a charge of +1) and be thereby converted into a corresponding neutrino (with a charge of 0), where the type ("flavour") of neutrino (electron ν e, muon ν μ, or tau ν τ) is the same as the type of lepton in the interaction, for example: + +

  9. Nuclear chemistry - Wikipedia

    en.wikipedia.org/wiki/Nuclear_chemistry

    11 C, carbon-11 is usually produced by cyclotron bombardment of 14 N with protons. The resulting nuclear reaction is 14 N(p,α) 11 C. [36] Additionally, carbon-11 can also be made using a cyclotron; boron in the form of boric oxide is reacted with protons in a (p,n) reaction. Another alternative route is to react 10 B with deuterons.