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  2. Neutron capture - Wikipedia

    en.wikipedia.org/wiki/Neutron_capture

    Neutron capture is a nuclear reaction in which an atomic nucleus and one or more neutrons collide and merge to form a heavier nucleus. [1] Since neutrons have no electric charge, they can enter a nucleus more easily than positively charged protons , which are repelled electrostatically .

  3. Neutron capture nucleosynthesis - Wikipedia

    en.wikipedia.org/wiki/Neutron_capture_nucleo...

    Neutron capture nucleosynthesis describes two nucleosynthesis pathways: the r-process and the s-process, for rapid and slow neutron captures, respectively. R-process describes neutron capture in a region of high neutron flux , such as during supernova nucleosynthesis after core-collapse, and yields neutron-rich nuclides .

  4. s-process - Wikipedia

    en.wikipedia.org/wiki/S-process

    The slow neutron-capture process, or s-process, is a series of reactions in nuclear astrophysics that occur in stars, particularly asymptotic giant branch stars. The s -process is responsible for the creation ( nucleosynthesis ) of approximately half the atomic nuclei heavier than iron .

  5. Photodisintegration - Wikipedia

    en.wikipedia.org/wiki/Photodisintegration

    Photodisintegration (also called phototransmutation, or a photonuclear reaction) is a nuclear process in which an atomic nucleus absorbs a high-energy gamma ray, enters an excited state, and immediately decays by emitting a subatomic particle.

  6. r-process - Wikipedia

    en.wikipedia.org/wiki/R-process

    In nuclear astrophysics, the rapid neutron-capture process, also known as the r-process, is a set of nuclear reactions that is responsible for the creation of approximately half of the atomic nuclei heavier than iron, the "heavy elements", with the other half produced by the p-process and s-process.

  7. Photofission - Wikipedia

    en.wikipedia.org/wiki/Photofission

    Photofission is a process in which a nucleus, after absorbing a gamma ray, undergoes nuclear fission and splits into two or more fragments.. The reaction was discovered in 1940 by a small team of engineers and scientists operating the Westinghouse Atom Smasher at the company's Research Laboratories in Forest Hills, Pennsylvania. [1]

  8. Nuclear medicine - Wikipedia

    en.wikipedia.org/wiki/Nuclear_medicine

    β + = β + decay; β − = β − decay; IT = isomeric transition; ec = electron capture * X-rays from progeny, mercury , Hg A typical nuclear medicine study involves administration of a radionuclide into the body by intravenous injection in liquid or aggregate form, ingestion while combined with food, inhalation as a gas or aerosol, or rarely ...

  9. Nuclear drip line - Wikipedia

    en.wikipedia.org/wiki/Nuclear_drip_line

    The boundaries of this valley are the neutron drip line on the neutron-rich side, and the proton drip line on the proton-rich side. [2] These limits exist because of particle decay, whereby an exothermic nuclear transition can occur by the emission of one or more nucleons (not to be confused with particle decay in particle physics).