Page 347 - Instant notes
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I6
                      ELECTRONIC SPECTROSCOPY



        Key Notes
                                The separation of energy levels arising from different
                                configurations of electrons in atomic and molecular orbitals
                                usually corresponds to radiation in the visible and ultraviolet
                                regions of the electromagnetic spectrum (wavelengths between
                                700 and ~100 nm).
                                Nuclei are sufficiently more massive than electrons that an
                                electronic transition (electron rearrangement) occurs so fast that
                                the nuclei do not alter their relative positions during the
                                transition.
                                The excitation of an electron from the π bonding orbital of a C=C
                                bond to the π* antibonding orbital is called a π−π* transition. The
                                excitation of one of the lone pair electrons of the O atom in a
                                C=O bond to the π* antibonding orbital is called an n−π*
                                transition. The energy of π−π* and n−π* transitions shifts to
                                longer wavelength radiation as conjugation of the C=C and C=O
                                bonds increases. A charge transfer transition involves electron
                                movement between the d orbital of a metal atom and a ligand.
                                Fluorescence is the emission of radiation directly following
                                absorption of excitation radiation. It is usually shifted to
                                frequencies lower than the absorption because some vibrational
                                excitation is lost in molecular collisions. Phosphorescence is the
                                slow emission of radiation after absorption ceases and usually
                                emanates from a triplet state accessed by spin-forbidden
                                intersystem crossing from the initial excited singlet state.
                                A photoelectron spectrum is obtained by measuring the kinetic
                                energies of electrons emitted from a molecule following
                                absorption of high energy (ultraviolet or X-ray) monochromatic
                                radiation. The difference between the energy of the incident
                                photon and the kinetic energy yields the energy of the orbital
                                from which the electron was ejected.
         Related topics         Valence bond theory (H2)   General features of
                                                         spectroscopy (I1)
                                Molecular orbital theory of
                                diatomic molecules I (H3)
                                                         Practical aspects of
                                                         spectroscopy (I2)
                                Molecular orbital theory of
                                diatomic molecules II (H4)
                                                         Photochemistry in the real
                                                         world (I7)
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