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Titlebook: Current Developments in Atomic, Molecular, and Chemical Physics with Applications; Man Mohan Book 2002 Springer Science+Business Media New

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樓主: decoction
51#
發(fā)表于 2025-3-30 12:16:49 | 只看該作者
Quantum Dynamics of Polyatomic MoleculesUntil very recently chemical dynamics was confined to few-atom systems. It is now state-of-art for small polyatomics (e.g. for triatomic and tetraatomic systems) and typically provide results far superior in precision and experimental relevance using classical molecular dynamics. Efforts are current
52#
發(fā)表于 2025-3-30 15:03:20 | 只看該作者
Study of the excited state dynamics to improve the optical limiting performance of tetra tolyl porpherials in general and metallo-porphyrins/related compounds in particular. The interest in metallo-porphyrins is many-fold. These molecules are found to have strong nonlinearity and fast response times, the desired criteria for making useful photonic devices. Previous theoretical and experimental stu
53#
發(fā)表于 2025-3-30 18:05:11 | 只看該作者
54#
發(fā)表于 2025-3-30 22:48:30 | 只看該作者
55#
發(fā)表于 2025-3-31 03:39:33 | 只看該作者
Theory and Control of Photo-excited Polyatomic Reactionsore excitation, the internal energy distribution of the molecule is the equilibrium Boltzmann distribution. The fate of this distribution after photo-excitation of the molecule from a ground electronic state (S.) to an excited electronic state (S.) has been rather ignored. The nature of the nascent
56#
發(fā)表于 2025-3-31 07:34:23 | 只看該作者
Van der Waals Interaction Probed by Solvatochromic Shiftsolvent interaction leads to changes in the molecular solute affecting its spectroscopic, structural and reactive properties. For this reason, the study of solvent effects has been a topic of increased interest.,.. UV-Vis absorption spectrum is very sensitive to solvent effects and it can thus be use
57#
發(fā)表于 2025-3-31 13:06:03 | 只看該作者
58#
發(fā)表于 2025-3-31 15:46:00 | 只看該作者
UV Spectroscopy by Electron Impact for Planetary Astronomy and Astrophysicsto measure electron impact emission cross sections (0-2keV) and fluorescence spectra (50-1200nm) for important atoms and molecules of planetary atmospheres, stellar atmospheres and the interstellar medium (ISM) for modeling remote sensing observations of EUVE, FUSE, HST, HUT, Galileo, Cassini and ma
59#
發(fā)表于 2025-3-31 18:49:29 | 只看該作者
60#
發(fā)表于 2025-4-1 01:11:02 | 只看該作者
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