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  2. Binding energy - Wikipedia

    en.wikipedia.org/wiki/Binding_energy

    Electron binding energy, more commonly known as ionization energy, [3] is a measure of the energy required to free an electron from its atomic orbital or from a solid. The electron binding energy derives from the electromagnetic interaction of the electron with the nucleus and the other electrons of the atom , molecule or solid and is mediated ...

  3. Bond energy - Wikipedia

    en.wikipedia.org/wiki/Bond_energy

    The bond dissociation energy (enthalpy) [4] is also referred to as bond disruption energy, bond energy, bond strength, or binding energy (abbreviation: BDE, BE, or D). It is defined as the standard enthalpy change of the following fission: R—X → R + X. The BDE, denoted by Dº(R—X), is usually derived by the thermochemical equation,

  4. Atomic physics - Wikipedia

    en.wikipedia.org/wiki/Atomic_physics

    The energy necessary to remove an electron from its shell (taking it to infinity) is called the binding energy. Any quantity of energy absorbed by the electron in excess of this amount is converted to kinetic energy according to the conservation of energy. The atom is said to have undergone the process of ionization.

  5. Valley of stability - Wikipedia

    en.wikipedia.org/wiki/Valley_of_stability

    The binding energy is subtracted from the sum of the proton and neutron masses because the mass of the nucleus is less than that sum. This property, called the mass defect, is necessary for a stable nucleus; within a nucleus, the nuclides are trapped by a potential well. A semi-empirical mass formula states that the binding energy will take the ...

  6. Nuclear structure - Wikipedia

    en.wikipedia.org/wiki/Nuclear_structure

    Difference between experimental binding energies and the liquid drop model prediction as a function of neutron number for Z>7. Systematic measurements of the binding energy of atomic nuclei show systematic deviations with respect to those estimated from the liquid drop model. In particular, some nuclei having certain values for the number of ...

  7. Island of stability - Wikipedia

    en.wikipedia.org/wiki/Island_of_stability

    The binding energy per nucleon increases with atomic number to a broad plateau around A = 60, then declines. [15] If a nucleus can be split into two parts that have a lower total energy (a consequence of the mass defect resulting from greater binding energy), it is unstable.

  8. Cation–π interaction - Wikipedia

    en.wikipedia.org/wiki/Cation–π_interaction

    The following table shows a series of Gibbs free energy of binding between benzene and several cations in the gas phase. [ 2 ] [ 6 ] For a singly charged species, the gas-phase interaction energy correlates with the ionic radius , r i o n {\displaystyle r_{\mathrm {ion} }} (non-spherical ionic radii are approximate).

  9. Semi-empirical mass formula - Wikipedia

    en.wikipedia.org/wiki/Semi-empirical_mass_formula

    Magnitude of the pairing term in the total binding energy for even–even and odd–odd nuclei, as a function of mass number. Two fits are shown (blue and red line). The pairing term (positive for even–even and negative for odd–odd nuclei) was derived from binding energy data. [6]

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