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  2. Neutrino - Wikipedia

    en.wikipedia.org/wiki/Neutrino

    The neutrino [a] was postulated first by Wolfgang Pauli in 1930 to explain how beta decay could conserve energy, momentum, and angular momentum ().In contrast to Niels Bohr, who proposed a statistical version of the conservation laws to explain the observed continuous energy spectra in beta decay, Pauli hypothesized an undetected particle that he called a "neutron", using the same -on ending ...

  3. Neutron - Wikipedia

    en.wikipedia.org/wiki/Neutron

    The number of neutrons is the neutron number. Neutrons do not affect the electron configuration. Atoms of a chemical element that differ only in neutron number are called isotopes. For example, carbon, with atomic number 6, has an abundant isotope carbon-12 with 6 neutrons and a rare isotope carbon-13 with 7 neutrons.

  4. Electron neutrino - Wikipedia

    en.wikipedia.org/wiki/Electron_neutrino

    Namely [there is] the possibility that there could exist in the nuclei electrically neutral particles that I wish to call neutrons, [b] which have spin ⁠ 1 / 2 ⁠ and obey the exclusion principle, and additionally differ from light quanta in that they do not travel with the velocity of light: The mass of the neutron must be of the same order ...

  5. Nuclear magnetic moment - Wikipedia

    en.wikipedia.org/wiki/Nuclear_magnetic_moment

    According to the shell model, protons or neutrons tend to form pairs of opposite total angular momentum.Therefore, the magnetic moment of a nucleus with even numbers of each protons and neutrons is zero, while that of a nucleus with an odd number of protons and even number of neutrons (or vice versa) will have to be that of the remaining unpaired nucleon.

  6. Even and odd atomic nuclei - Wikipedia

    en.wikipedia.org/wiki/Even_and_odd_atomic_nuclei

    ; spins 1, 1, 3, 1). All four of these isotopes have the same number of protons and neutrons, and they all have an odd number for their nuclear spin. The only other observationally "stable" odd–odd nuclide is 180m 73 Ta (spin 9), the only primordial nuclear isomer, which has not yet been observed to decay despite experimental attempts. [5]

  7. Electron - Wikipedia

    en.wikipedia.org/wiki/Electron

    If a body has more or fewer electrons than are required to balance the positive charge of the nuclei, then that object has a net electric charge. When there is an excess of electrons, the object is said to be negatively charged. When there are fewer electrons than the number of protons in nuclei, the object is said to be positively charged.

  8. Atomic nucleus - Wikipedia

    en.wikipedia.org/wiki/Atomic_nucleus

    The stable nucleus has approximately a constant density and therefore the nuclear radius R can be approximated by the following formula, = / 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.

  9. Atom - Wikipedia

    en.wikipedia.org/wiki/Atom

    If an atom has more electrons than protons, then it has an overall negative charge, and is called a negative ion (or anion). Conversely, if it has more protons than electrons, it has a positive charge, and is called a positive ion (or cation). The electrons of an atom are attracted to the protons in an atomic nucleus by the electromagnetic force.