標(biāo)題: Titlebook: Autoionization; Recent Developments Aaron Temkin Book 1985 Springer Science+Business Media New York 1985 Corona.autoionization.development [打印本頁(yè)] 作者: 反抗日本 時(shí)間: 2025-3-21 18:37
書目名稱Autoionization影響因子(影響力)
書目名稱Autoionization影響因子(影響力)學(xué)科排名
書目名稱Autoionization網(wǎng)絡(luò)公開度
書目名稱Autoionization網(wǎng)絡(luò)公開度學(xué)科排名
書目名稱Autoionization被引頻次
書目名稱Autoionization被引頻次學(xué)科排名
書目名稱Autoionization年度引用
書目名稱Autoionization年度引用學(xué)科排名
書目名稱Autoionization讀者反饋
書目名稱Autoionization讀者反饋學(xué)科排名
作者: 溫和女孩 時(shí)間: 2025-3-21 23:24 作者: 防御 時(shí)間: 2025-3-22 02:40
Hole-Projection Method for Calculating Feshbach Resonances and Inner-Shell Vacancies,t is embedded in the continuum. In most cases, they are coupled to the continuum via the Coulomb interaction, although this coupling may be very weak, so that the energy level and wave function can be obtained approximately by using square-integrable basis functions. This coupling can cause consider作者: 不近人情 時(shí)間: 2025-3-22 05:03 作者: 期滿 時(shí)間: 2025-3-22 11:17
Molecular Resonance Calculations Applications of Complex-Coordinate and Complex Basis Function Techize from H. to naphthalene (C.H.). In fact, almost every organic molecule containing a double bond displays at least one low-energy resonance.. The mechanism of formation for these low-energy resonances can be viewed in two superficially different, but essentially equivalent, ways, depending on whet作者: addict 時(shí)間: 2025-3-22 14:25
Diagnostics of Solar and Astrophysical Plasmas Dependent on Autoionization Phenomena,hen incorporated into spectroscopic diagnostic tools used to determine physical conditions in astrophysical plasmas. The discussion here is limited to the interpretation of spectral line intensities at ultraviolet and shorter wavelengths, and, therefore, the corresponding emphasis is on calculations作者: interlude 時(shí)間: 2025-3-22 17:25
Gesund und fit in der zweiten Lebensh?lfteher we initially adopt the point of view of the atomic physicist or quantum chemist. From both points of view, most of the resonances below 5-eV incident energy in electron-molecule scattering can be thought of in the first approximation as “shape” resonances, that is, not involving electronic excitation of the target molecule.作者: 寵愛(ài) 時(shí)間: 2025-3-22 21:33
Molecular Resonance Calculations Applications of Complex-Coordinate and Complex Basis Function Techher we initially adopt the point of view of the atomic physicist or quantum chemist. From both points of view, most of the resonances below 5-eV incident energy in electron-molecule scattering can be thought of in the first approximation as “shape” resonances, that is, not involving electronic excitation of the target molecule.作者: orient 時(shí)間: 2025-3-23 02:37
Gesund und fit in der zweiten Lebensh?lfterable precision arises from two causes: not only can we not give the exact eigenfunctions analytically, but we cannot even supply a formal, explicit expression for the projection operators that we need at the outset.作者: 鎮(zhèn)壓 時(shí)間: 2025-3-23 06:04 作者: 協(xié)迫 時(shí)間: 2025-3-23 10:35 作者: flavonoids 時(shí)間: 2025-3-23 17:36
Projection and Quasi-Projection Operators for Electron Impact Resonances on Many-Electron Atomic Tarable precision arises from two causes: not only can we not give the exact eigenfunctions analytically, but we cannot even supply a formal, explicit expression for the projection operators that we need at the outset.作者: GRIEF 時(shí)間: 2025-3-23 19:51
Hole-Projection Method for Calculating Feshbach Resonances and Inner-Shell Vacancies,ure, etc. Once formed, they may decay by inner-shell or outer-shell autoionization, Coster-Kronig transition, x-ray emission, etc.. The application of these effects covers a wide range of disciplines in physics and electronics as well as medical and geophysical sciences.作者: conformity 時(shí)間: 2025-3-23 23:18 作者: 規(guī)章 時(shí)間: 2025-3-24 05:05 作者: 高度贊揚(yáng) 時(shí)間: 2025-3-24 06:50
Gesund und fit in der zweiten Lebensh?lftea target ion or atom. They can also be produced by photoabsorption as well as heavy-particle collisions. It is only comparatively recently that such resonances have been studied in great detail as a result of important experimental and theoretical developments together with the advent of high-speed computers.作者: 金絲雀 時(shí)間: 2025-3-24 14:30
Theory and Calculation of Resonances and Autoionization of Two-Electron Atoms and Ions,a target ion or atom. They can also be produced by photoabsorption as well as heavy-particle collisions. It is only comparatively recently that such resonances have been studied in great detail as a result of important experimental and theoretical developments together with the advent of high-speed computers.作者: 大門在匯總 時(shí)間: 2025-3-24 15:58 作者: JOG 時(shí)間: 2025-3-24 19:41 作者: Irremediable 時(shí)間: 2025-3-25 01:42 作者: 玉米 時(shí)間: 2025-3-25 05:40 作者: 親屬 時(shí)間: 2025-3-25 11:20 作者: 意外 時(shí)間: 2025-3-25 15:31
Physics of Atoms and Moleculeshttp://image.papertrans.cn/b/image/166163.jpg作者: 親密 時(shí)間: 2025-3-25 16:18 作者: MOCK 時(shí)間: 2025-3-25 20:10 作者: ablate 時(shí)間: 2025-3-26 01:37
Gesund und fit in der zweiten Lebensh?lfteelectron autoionization systems (implying a one-electron target) was given in Chapter 1; to repeat briefly, the fact that the target eigenfunctions are known analytically and the special character of a one-electron target allow exact projection operators in the Feshbach sense. to be written down, wh作者: PRO 時(shí)間: 2025-3-26 08:11 作者: 并置 時(shí)間: 2025-3-26 11:50 作者: BIPED 時(shí)間: 2025-3-26 13:56 作者: expdient 時(shí)間: 2025-3-26 17:48
Gesund und fit in der zweiten Lebensh?lftehen incorporated into spectroscopic diagnostic tools used to determine physical conditions in astrophysical plasmas. The discussion here is limited to the interpretation of spectral line intensities at ultraviolet and shorter wavelengths, and, therefore, the corresponding emphasis is on calculations作者: 負(fù)擔(dān) 時(shí)間: 2025-3-26 22:57
Diagnostics of Solar and Astrophysical Plasmas Dependent on Autoionization Phenomena,hen incorporated into spectroscopic diagnostic tools used to determine physical conditions in astrophysical plasmas. The discussion here is limited to the interpretation of spectral line intensities at ultraviolet and shorter wavelengths, and, therefore, the corresponding emphasis is on calculations involving highly ionized atoms.作者: BLAZE 時(shí)間: 2025-3-27 03:57
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