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  2. Neutrino - Wikipedia

    en.wikipedia.org/wiki/Neutrino

    A neutrino (/ njuːˈtriːnoʊ / new-TREE-noh; denoted by the Greek letter ν) is a fermion (an elementary particle with spin of ⁠ 1 2 ⁠) that interacts only via the weak interaction and gravity. [2][3] The neutrino is so named because it is electrically neutral and because its rest mass is so small (-ino) that it was long thought to be zero.

  3. Nuclear binding energy - Wikipedia

    en.wikipedia.org/wiki/Nuclear_binding_energy

    Nuclear binding energy in experimental physics is the minimum energy that is required to disassemble the nucleus of an atom into its constituent protons and neutrons, known collectively as nucleons. The binding energy for stable nuclei is always a positive number, as the nucleus must gain energy for the nucleons to move apart from each other.

  4. Neutrino decoupling - Wikipedia

    en.wikipedia.org/wiki/Neutrino_decoupling

    Neutrino decoupling. In Big Bang cosmology, neutrino decoupling was the epoch at which neutrinos ceased interacting with other types of matter, [1] and thereby ceased influencing the dynamics of the universe at early times. [2] Prior to decoupling, neutrinos were in thermal equilibrium with protons, neutrons and electrons, which was maintained ...

  5. List of equations in nuclear and particle physics - Wikipedia

    en.wikipedia.org/wiki/List_of_equations_in...

    Mass number. A = (Relative) atomic mass = Mass number = Sum of protons and neutrons. N = Number of neutrons. Z = Atomic number = Number of protons = Number of electrons. A = Z + N {\displaystyle A=Z+N\,\!} Mass in nuclei. M'nuc = Mass of nucleus, bound nucleons. MΣ = Sum of masses for isolated nucleons.

  6. Neutron - Wikipedia

    en.wikipedia.org/wiki/Neutron

    An atomic nucleus is formed by a number of protons, Z (the atomic number), and a number of neutrons, N (the neutron number), bound together by the nuclear force. Protons and neutrons each have a mass of approximately one dalton. The atomic number determines the chemical properties of the atom, and the neutron number determines the isotope or ...

  7. Atomic nucleus - Wikipedia

    en.wikipedia.org/wiki/Atomic_nucleus

    where A = Atomic mass number (the number of protons Z, plus the number of neutrons N) and r 0 = 1.25 fm = 1.25 × 10 −15 m. In this equation, the "constant" r 0 varies by 0.2 fm, depending on the nucleus in question, but this is less than 20% change from a constant.

  8. Neutron transport - Wikipedia

    en.wikipedia.org/wiki/Neutron_transport

    v. t. e. Neutron transport (also known as neutronics) is the study of the motions and interactions of neutrons with materials. Nuclear scientists and engineers often need to know where neutrons are in an apparatus, in what direction they are going, and how quickly they are moving.

  9. Helium atom - Wikipedia

    en.wikipedia.org/wiki/Helium_atom

    Helium is composed of two electrons bound by the electromagnetic force to a nucleus containing two protons along with two neutrons, depending on the isotope, held together by the strong force. Unlike for hydrogen , a closed-form solution to the Schrödinger equation for the helium atom has not been found.

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