CHEM 1300 Chapter Notes - Chapter 5 : Pauli Exclusion Principle, Noble Gas, Diamagnetism

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5. 1 - orbital energies: as the number of n and l goes up, the orbital energy goes up, orbital energies also depends on the attraction between the electrons in the orbital and the protons in the nucleus. How much are those protons pulling those electrons : hydrogen absorbs light > energy of photon goes from ground state to excited state. Thus moving the electron to larger less stable orbital. Photoelectron spectroscopy pes: works with gases instead of metals, energy of various orbitals can be calculated thru the energy of the incoming photon and the. Ionization energy: it is the amount of energy required to remove an electron from an atom/ion. Positively charged = higher ionization energy than neutral. Multi-electron system, electrons repel each other thus decreasing ionization energy. Screening: electrons approach positive cation, other electrons repel it, and the nucleus attracts it. known as screening.

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