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  2. Neutron - Wikipedia

    en.wikipedia.org/wiki/Neutron

    Neutrons are required for the stability of nuclei, with the exception of the single-proton hydrogen nucleus. Neutrons are produced copiously in nuclear fission and fusion. They are a primary contributor to the nucleosynthesis of chemical elements within stars through fission, fusion, and neutron capture processes.

  3. Atomic nucleus - Wikipedia

    en.wikipedia.org/wiki/Atomic_nucleus

    Protons define the entire charge of a nucleus, and hence its chemical identity. Neutrons are electrically neutral, but contribute to the mass of a nucleus to nearly the same extent as the protons. Neutrons can explain the phenomenon of isotopes (same atomic number with different atomic mass). The main role of neutrons is to reduce electrostatic ...

  4. Atomic number - Wikipedia

    en.wikipedia.org/wiki/Atomic_number

    The atomic number or nuclear charge number (symbol Z) of a chemical element is the charge number of its atomic nucleus. For ordinary nuclei composed of protons and neutrons , this is equal to the proton number ( n p ) or the number of protons found in the nucleus of every atom of that element.

  5. Nucleon - Wikipedia

    en.wikipedia.org/wiki/Nucleon

    The proton carries a positive net charge, and the neutron carries a zero net charge; the proton's mass is only about 0.13% less than the neutron's. Thus, they can be viewed as two states of the same nucleon, and together form an isospin doublet (I = ⁠ 1 / 2 ⁠). In isospin space, neutrons can be transformed into protons and conversely by SU ...

  6. Proton - Wikipedia

    en.wikipedia.org/wiki/Proton

    Since the atomic number of hydrogen is 1, a hydrogen ion has no electrons and corresponds to a bare nucleus, consisting of a proton (and 0 neutrons for the most abundant isotope protium 1 1 H). The proton is a "bare charge" with only about 1/64,000 of the radius of a hydrogen atom, and so is extremely reactive chemically.

  7. Free neutron decay - Wikipedia

    en.wikipedia.org/wiki/Free_neutron_decay

    For the free neutron, the decay energy for this process (based on the rest masses of the neutron, proton and electron) is 0.782 343 MeV.That is the difference between the rest mass of the neutron and the sum of the rest masses of the products.

  8. Plutonium-240 - Wikipedia

    en.wikipedia.org/wiki/Plutonium-240

    Decay chain of 240 Pu. Plutonium-240 (240 Pu or Pu-240) is an isotope of plutonium formed when plutonium-239 captures a neutron.The detection of its spontaneous fission led to its discovery in 1944 at Los Alamos and had important consequences for the Manhattan Project.

  9. Neutron radiation - Wikipedia

    en.wikipedia.org/wiki/Neutron_radiation

    Neutron radiation is a form of ionizing radiation that presents as free neutrons.Typical phenomena are nuclear fission or nuclear fusion causing the release of free neutrons, which then react with nuclei of other atoms to form new nuclides—which, in turn, may trigger further neutron radiation.