When.com Web Search

Search results

  1. Results From The WOW.Com Content Network
  2. Pauli exclusion principle - Wikipedia

    en.wikipedia.org/wiki/Pauli_exclusion_principle

    In that case, the two values of m s (spin) pair must be different. Since the only two possible values for the spin projection m s are +1/2 and −1/2, it follows that one electron must have m s = +1/2 and one m s = −1/2. Particles with an integer spin are not subject to the Pauli exclusion principle

  3. Electron pair - Wikipedia

    en.wikipedia.org/wiki/Electron_pair

    In both cases a bond is created by the formation of an electron pair. Because electrons are fermions, the Pauli exclusion principle forbids these particles from having all the same quantum numbers. Therefore, for two electrons to occupy the same orbital, and thereby have the same orbital quantum number, they must have different spin quantum numbers

  4. Pauli matrices - Wikipedia

    en.wikipedia.org/wiki/Pauli_matrices

    Wolfgang Pauli (1900–1958), c. 1924. Pauli received the Nobel Prize in Physics in 1945, nominated by Albert Einstein, for the Pauli exclusion principle.. In mathematical physics and mathematics, the Pauli matrices are a set of three 2 × 2 complex matrices that are traceless, Hermitian, involutory and unitary.

  5. Exchange interaction - Wikipedia

    en.wikipedia.org/wiki/Exchange_interaction

    Although these consequences of the exchange interaction are magnetic in nature, the cause is not; it is due primarily to electric repulsion and the Pauli exclusion principle. In general, the direct magnetic interaction between a pair of electrons (due to their electron magnetic moments) is negligibly small compared to this electric interaction.

  6. Degenerate matter - Wikipedia

    en.wikipedia.org/wiki/Degenerate_matter

    The electron gas in ordinary metals and in the interior of white dwarfs are two examples. Following the Pauli exclusion principle, there can be only one fermion occupying each quantum state. In a degenerate gas, all quantum states are filled up to the Fermi energy.

  7. Nuclear structure - Wikipedia

    en.wikipedia.org/wiki/Nuclear_structure

    The terms proportional to and / represent the volume and surface energy of the liquid drop, the term proportional to represents the electrostatic energy, the term proportional to () represents the Pauli exclusion principle and the last term (,) is the pairing term, which lowers the energy for even numbers of protons or neutrons.

  8. Nuclear shell model - Wikipedia

    en.wikipedia.org/wiki/Nuclear_shell_model

    The same is true for neutrons. All protons in the same level (n) have the same parity (either +1 or −1), and since the parity of a pair of particles is the product of their parities, an even number of protons from the same level (n) will have +1 parity. Thus, the total angular momentum of the eight protons and the first eight neutrons is zero ...

  9. Shape of the atomic nucleus - Wikipedia

    en.wikipedia.org/wiki/Shape_of_the_atomic_nucleus

    The exclusion principle is built into the anti-symmetric fermionic wave function, thereby forbidding a pair of identical fermions from occupying the same quantum state. [19] In accordance with Pauli exclusion force, [ dubious – discuss ] the spin-spin repulsive force between identical fermions pushes like-flavored quarks further apart.