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  2. Kaufmann–Bucherer–Neumann experiments - Wikipedia

    en.wikipedia.org/wiki/Kaufmann–Bucherer...

    [A 20] [A 21] [A 22] Lorentz summarized these efforts in 1915: [A 23] Later experiments [..] have confirmed the formula [..] for the transverse electromagnetic mass, so that, in all probability, the only objection that could be raised against the hypothesis of the deformable electron and the principle of relativity has now been removed.

  3. Effective nuclear charge - Wikipedia

    en.wikipedia.org/wiki/Effective_nuclear_charge

    In atomic physics, the effective nuclear charge of an electron in a multi-electron atom or ion is the number of elementary charges an electron experiences by the nucleus. It is denoted by Z eff . The term "effective" is used because the shielding effect of negatively charged electrons prevent higher energy electrons from experiencing the full ...

  4. Mass-to-charge ratio - Wikipedia

    en.wikipedia.org/wiki/Mass-to-charge_ratio

    When charged particles move in electric and magnetic fields the following two laws apply: Lorentz force law: = (+),; Newton's second law of motion: = =; where F is the force applied to the ion, m is the mass of the particle, a is the acceleration, Q is the electric charge, E is the electric field, and v × B is the cross product of the ion's velocity and the magnetic flux density.

  5. Electron - Wikipedia

    en.wikipedia.org/wiki/Electron

    Electron therapy can treat such skin lesions as basal-cell carcinomas because an electron beam only penetrates to a limited depth before being absorbed, typically up to 5 cm for electron energies in the range 520 MeV. An electron beam can be used to supplement the treatment of areas that have been irradiated by X-rays. [182] [183]

  6. Shape of the atomic nucleus - Wikipedia

    en.wikipedia.org/wiki/Shape_of_the_atomic_nucleus

    Electron scattering techniques have yielded clues as to the internal structure of light nuclides. Proton-neutron pairs experience a strongly repulsive component of the nuclear force within ≈ 0.5 fm (see "Space between nucleons" above). As nucleons cannot pack any closer, nearly all nuclei have the same central density. [6]

  7. Hubbard model - Wikipedia

    en.wikipedia.org/wiki/Hubbard_model

    The Hubbard model states that each electron experiences competing forces: one pushes it to tunnel to neighboring atoms, while the other pushes it away from its neighbors. [2] Its Hamiltonian thus has two terms: a kinetic term allowing for tunneling ("hopping") of particles between lattice sites and a potential term reflecting on-site interaction.

  8. Ponderomotive energy - Wikipedia

    en.wikipedia.org/wiki/Ponderomotive_energy

    where is the electron charge, is the linearly polarised electric field amplitude, is the laser carrier frequency and is the electron mass. In terms of the laser intensity I {\displaystyle I} , using I = c ϵ 0 E 2 / 2 {\displaystyle I=c\epsilon _{0}E^{2}/2} , it reads less simply:

  9. Shielding effect - Wikipedia

    en.wikipedia.org/wiki/Shielding_effect

    The wider the electron shells are in space, the weaker is the electric interaction between the electrons and the nucleus due to screening. Further, because of differences in orbital penetration, we can order the screening strength, S, that electrons in a given orbital (s, p, d, or f) provide to the rest of the electrons thusly: > > > ().