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VI. ELECTRONIC SPECTROSCOPY The visible (V) and ultraviolet
VI. ELECTRONIC SPECTROSCOPY The visible (V) and ultraviolet

... Two states of the same energy are mixed strongly if a perturbation is present, and hence the initial state can be nudged into the final state by even a weak perturbation. The perturbation that drives IC is the breakdown of the BO approximation, for the electrons do not exactly follow the changing lo ...
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... its atomic spectrum. In this model the energy of the hydrogen atom depends on its quantum number, (4). The value of n must be a positive integer (1, 2, 3, . . .) and each value of n corresponds to a different energy; En = (5). As n increases, the energy of the electron (6) until it reaches a value o ...
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... spectrometer, when electron energies are ≥ 4.86 eV. (It would be difficult to observe in air near normal incidence.) (The Hg atom, in its first excited state at 4.667 eV, cannot de-excite by radiation; as discussed above, angular momentum could not be conserved. The 3P0 state is metastable, drifting ...
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2 - TEST BANK 360
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... observing how a charged drop of oil falls in the presence and in the absence of an electric field. An atomizer introduces a fine mist of oil drops into the top chamber (Figure 2.6). Several drops happen to fall through a small hole into the lower chamber, where the experimenter follows the motion of ...
Regents Chemistry Topic Review Packet
Regents Chemistry Topic Review Packet

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... (4) located in a solid sphere covering the nucleus 3. An experiment in which alpha particles were used to bombard thin sheets of gold foil led to the conclusion that an atom is composed mostly of (1) empty space and has a small, negatively charged nucleus (2) empty space and has a small, positively ...
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O - gearju.com
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... (a) The electronegativity difference between H and Cl is 0.9, which is appreciable but not large enough (by the 2.0 rule) to qualify HCl as an ionic compound. Therefore, the bond between H and Cl is polar covalent. (b) The electronegativity difference between K and F is 3.2, which is well above the ...
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... special selection mechanism when forming molecules and clusters using this method: A helium droplet is an excellent heat bath at 380 mK. A large input of energy, e.g., the chemical binding energy set free upon molecule or cluster formation appears as local heat to be dissipated by massive evaporatio ...
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... II.3 Elements can be classified by their properties and located on the Periodic Table as metals, nonmetals, metalloids (B, Si, Ge, As, Sb, Te), and noble gases. (3.1v) II.4 Elements can be differentiated by their physical properties. Physical properties of substances, such as density, conductivity, ...
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... observing how a charged drop of oil falls in the presence and in the absence of an electric field. An atomizer introduces a fine mist of oil drops into the top chamber (Figure 2.6). Several drops happen to fall through a small hole into the lower chamber, where the experimenter follows the motion of ...
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International Journal of Quantum Chemistry 77, 871-879
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... free atom. The true interaction potential between valence electrons and atomic cores is replaced by an ab initio pseudopotential that has almost exactly the same scattering properties. The key property of the pseudopotential is that in the core region the resulting “pseudo-wave-functions” lack the r ...
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... with detailed observations of individual systems, in order to further the goal of making more detailed models of such systems, including triggering and termination of AGN heating. We describe here multi-wavelength observations of the X-ray cluster 2A0335+096 that illustrate how complex these interac ...
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Metastable inner-shell molecular state



Metastable Innershell Molecular State (MIMS) is a class of ultra-high-energy short-lived molecules have the binding energy up to 1,000 times larger and bond length up to 100 times smaller than typical molecules. MIMS is formed by inner-shell electrons that are normally resistant to molecular formation. However, in stellar conditions, the inner-shell electrons become reactive to form molecular structures (MIMS) from combinations of all elements in the periodic table. MIMS upon dissociation can emit x-ray photons with energies up to 100 keV at extremely high conversion efficiencies from compression energy to photon energy. MIMS is predicted to exist and dominate radiation processes in extreme astrophysical environments, such as large planet cores, star interiors, and black hole and neutron star surroundings. There, MIMS is predicted to enable highly energy-efficient transformation of the stellar compression energy into the radiation energy.The right schematic illustration shows the proposed four stages of the K-shell MIMS (K-MIMS) formation and x-ray generation process. Stage I: Individual atoms are subjected to the stellar compression and ready for absorbing the compression energy. Stage II: The outer electron shells fuse together under increasing ""stellar"" pressure. Stage III: At the peak pressure, via pressure ionization K-shell orbits form the K-MIMS, which is vibrationally hot and encapsulated by a Rydberg-like pseudo-L-Shell structure. Stage IV: The K-MIMS cools down by ionizing (""boiling-off"") a number of pseudo-L-shell electrons and subsequent optical decay by emitting an x-ray photon. The dissociated atoms return their original atoms states and are ready for absorbing the compression energy.MIMS also can be readily produced in laboratory and industrial environments, such as hypervelocity particle impact, laser fusion and z-machine. MIMS can be exploited for highly energy-efficient production of high intensity x-ray beams for a wide range of innovative applications, such as photolithography, x-ray lasers, and inertial fusion.
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