𝔖 Bobbio Scriptorium
✦   LIBER   ✦

A model of galactic cosmic rays for use in calculating linear energy transfer spectra

✍ Scribed by J. Chen; D. Chenette; R. Clark; M. Garcia-Munoz; T.G. Guzik; K.R. Pyle; Y. Sang; J.P. Wefel

Publisher
Elsevier Science
Year
1994
Tongue
English
Weight
373 KB
Volume
14
Category
Article
ISSN
0273-1177

No coin nor oath required. For personal study only.

πŸ“œ SIMILAR VOLUMES

A program for the calculation of energy
A program for the calculation of energy spectra and reduced nuclear matrix elements in the frame of the Davydov-Chaban model
✍ J. Lubian; R. Cabezas πŸ“‚ Article πŸ“… 1993 πŸ› Elsevier Science 🌐 English βš– 763 KB

In this code, the energy spectra of nuclei and the first-and second-order reduced nuclear matrix elements for coupled-channel calculations are computed. To describe the structure of the target nucleus, the Davydov-Chaban model, including quadrupole and hexadecapole modes, was used.

Use of semi-empirical models for calcula
Use of semi-empirical models for calculation of B terms in MCD spectra. PPP model for [4N + 2] annulenes: a rule for substituent and heteroatom effects
✍ Joseph Michl πŸ“‚ Article πŸ“… 1976 πŸ› Elsevier Science 🌐 English βš– 335 KB

UGng the PPP model at monocxcltcd CI level and scvcral addItIonal blmphfying assumptions, the sign and magnitude of the lowest hICD (mdgnetlc circular dichrolc) band of a [4N + 21 nnnulcnc of arbitrary six perturbed by one or more substitucnts and/or hctcroatoms nrc cvaluatcd in closed form and r&te