๐”– Bobbio Scriptorium
โœฆ   LIBER   โœฆ

An Orbital-Energy Well Model for Understanding Atomic Spectra

โœ Scribed by Stanley K. Derby

Book ID
114973893
Publisher
School Science and Mathematics Association
Year
1968
Tongue
English
Weight
87 KB
Volume
68
Category
Article
ISSN
0036-6803

No coin nor oath required. For personal study only.

๐Ÿ“œ SIMILAR VOLUMES

An atomic model for the spin-polarized p
An atomic model for the spin-polarized photoemission spectra of Fe
โœ P.S. Bagus; J.V. Mallow ๐Ÿ“‚ Article ๐Ÿ“… 1994 ๐Ÿ› Elsevier Science ๐ŸŒ English โš– 404 KB

Spin-polarized 3p and 3s photoemission spectra have been determined from ab initio wavefunctions for the ionized states of an isolated Fe + (3d 7) atomic ion. This ion is used to model the atomic effects which contribute to the core-level photoemission, including spin-polarization, from bulk Fe. We

An orbital hopping model for the calcula
An orbital hopping model for the calculation of intensity distributions of ionization spectra. The rotational linestrength distribution of NO ZEKE spectra
โœ V.M. Akulin; G. Reiser; E.W. Schlag ๐Ÿ“‚ Article ๐Ÿ“… 1992 ๐Ÿ› Elsevier Science ๐ŸŒ English โš– 437 KB

We present a new approach for understanding rotational linestrength distributions in ZEKE spectra of NO. A model is described in which orbital hopping of an electron is induced by scattering at the ion core. For diatomic molecules the intensity distribution only depends on an effective interatomic d