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  2. Binding energy - Wikipedia

    en.wikipedia.org/wiki/Binding_energy

    The atomic binding energy of the atom is the energy required to disassemble an atom into free electrons and a nucleus. [4] It is the sum of the ionization energies of all the electrons belonging to a specific atom. The atomic binding energy derives from the electromagnetic interaction of the electrons with the nucleus, mediated by photons.

  3. Activation energy - Wikipedia

    en.wikipedia.org/wiki/Activation_energy

    This is possible due to a release of energy that occurs when the substrate binds to the active site of a catalyst. This energy is known as Binding Energy. Upon binding to a catalyst, substrates partake in numerous stabilizing forces while within the active site (e.g. hydrogen bonding or van der Waals forces). Specific and favorable bonding ...

  4. Category:Binding energy - Wikipedia

    en.wikipedia.org/wiki/Category:Binding_energy

    Download as PDF; Printable version; In other projects Wikidata item; ... Pages in category "Binding energy" The following 9 pages are in this category, out of 9 total.

  5. Semi-empirical mass formula - Wikipedia

    en.wikipedia.org/wiki/Semi-empirical_mass_formula

    Coulomb energy, the potential energy from each pair of protons. As this is a repelling force, the binding energy is reduced. Asymmetry energy (also called Pauli energy), which accounts for the Pauli exclusion principle. Unequal numbers of neutrons and protons imply filling higher energy levels for one type of particle, while leaving lower ...

  6. File:Binding energy curve - common isotopes with gridlines.svg

    en.wikipedia.org/wiki/File:Binding_energy_curve...

    English: See the original work Image:Binding energy curve - common isotopes.svg for more information. This image just has the gridlines extended all the way up to the top. This image just has the gridlines extended all the way up to the top.

  7. Gravitational binding energy - Wikipedia

    en.wikipedia.org/wiki/Gravitational_binding_energy

    Using this, the real gravitational binding energy of Earth can be calculated numerically as U = 2.49 × 10 32 J. According to the virial theorem, the gravitational binding energy of a star is about two times its internal thermal energy in order for hydrostatic equilibrium to be maintained. [2]

  8. 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.

  9. Interaction energy - Wikipedia

    en.wikipedia.org/wiki/Interaction_energy

    In physics, interaction energy is the contribution to the total energy that is caused by an interaction between the objects being considered.. The interaction energy usually depends on the relative position of the objects.