{"id":6017,"date":"2021-09-28T17:37:24","date_gmt":"2021-09-28T15:37:24","guid":{"rendered":"http:\/\/fs.ummto.dz\/?p=6017"},"modified":"2021-11-29T08:32:16","modified_gmt":"2021-11-29T07:32:16","slug":"avis-de-soutenance-de-doctorat-de-3eme-cycle-en-physique","status":"publish","type":"post","link":"https:\/\/www.ummto.dz\/fs\/avis-de-soutenance-de-doctorat-de-3eme-cycle-en-physique\/","title":{"rendered":"Avis de Soutenance de doctorat en Physique de Anis CHIKH le 03\/10\/2021"},"content":{"rendered":"

Monsieur CHIKH Anis<\/span> soutiendra sa th\u00e8se de doctorat 3\u00e8me cycle\u00a0 en physique, intitul\u00e9e:<\/strong><\/p>\n

\u00a0Etude des propri\u00e9t\u00e9s radiatives d\u2019ions de terres rares\u00a0: cas des ions Er3+<\/sup>, Dy3+<\/sup> et Ho3+\u00a0<\/sup><\/strong><\/span><\/span><\/p>\n

Date de soutenance<\/strong><\/span><\/span>: 03 octobre 2021<\/span><\/strong><\/p>\n

Lieu de soutenance<\/span>:<\/strong> Salle de visioconf\u00e9rence du centre des syst\u00e8mes et r\u00e9seaux (Campus Bastos).<\/span><\/strong><\/span><\/p>\n

Jury de soutenance<\/span>:<\/strong><\/span><\/p>\n\n\n\n\n\n\n\n\n
Nom et Pr\u00e9nom<\/span><\/strong><\/td>\nGrade<\/span><\/strong><\/td>\nLieu d\u2019exercice<\/span><\/strong><\/td>\nQualit\u00e9<\/span><\/strong><\/td>\n<\/tr>\n
ZIANE Abdelhamid<\/span><\/td>\nProfesseur<\/span><\/td>\nUMMTO<\/span><\/td>\nPr\u00e9sident<\/span><\/td>\n<\/tr>\n
DEGHICHE Djamel<\/span><\/td>\nMCA<\/span><\/td>\nUMMTO<\/span><\/td>\nRapporteur<\/span><\/td>\n<\/tr>\n
TCHANG-BRILLET Lydia<\/span><\/td>\nProfesseur<\/span><\/td>\nSorbonne universit\u00e9<\/span><\/td>\nCo-Rapporteur<\/span><\/td>\n<\/tr>\n
GHERBI Abdelhakim<\/span><\/td>\nProfesseur<\/span><\/td>\nUAMB<\/span><\/td>\nExaminateur<\/span><\/td>\n<\/tr>\n
AOUCHICHE Hocine<\/span><\/td>\nProfesseur<\/span><\/td>\nUMMTO<\/span><\/td>\nExaminateur<\/span><\/td>\n<\/tr>\n<\/tbody>\n<\/table>\n


\nR\u00e9sum\u00e9 de la th\u00e8se<\/span>:<\/strong><\/p>\n

Cette th\u00e8se porte sur l’\u00e9tude des propri\u00e9t\u00e9s spectroscopiques d’ions trivalents de terres rares, cas de Er3+,<\/sup> dy3+ <\/sup>et Ho3+.<\/sup> Pour l’ion ErIV, nous avons \u00e9tendu et analys\u00e9 le spectre ultraviolet sous vide (VUV) dans la r\u00e9gion allant de 705 \u00e0 2460 \u00c5 moyennant la m\u00e9thode param\u00e9trique de Racah-Slater impl\u00e9ment\u00e9e dans la s\u00e9rie des codes ab-initio<\/em>de R.D Cowan. Les spectres exp\u00e9rimentaux ont \u00e9t\u00e9 produits et enregistr\u00e9s avec le spectrographe de 10.7m de l’observatoire de Paris-Meudon. Ce qui nous a permis d’identifier 1022 nouvelles raies comme transitions entre les configurations f11<\/sup>, f10<\/sup>d, f10<\/sup>s, f10<\/sup>p additionn\u00e9es aux 591 raies identifi\u00e9es pr\u00e9c\u00e9demment. Ces identifications ont eu pour effet de d\u00e9terminer 168 nouveaux niveaux d’\u00e9nergie de l’ErIV pour une d\u00e9viation moyenne de 51 cm-1<\/sup> pour les configurations impaires (f11<\/sup> et f10<\/sup>p) et de 53cm-1<\/sup> pour les configurations paires (f10<\/sup>d et f10<\/sup>s). Le nombre important de niveaux exp\u00e9rimentaux identifi\u00e9s donne une meilleure d\u00e9finition des param\u00e8tres de Racah, ce qui am\u00e9liore la pr\u00e9diction des niveaux inconnus et les probabilit\u00e9s de transitions.<\/span><\/p>\n

Pour le Dy3+<\/sup>et le Ho3+<\/sup>, nous nous sommes int\u00e9ress\u00e9s \u00e0 l’\u00e9tude th\u00e9orique des propri\u00e9t\u00e9s radiatives en utilisant les facteurs d’\u00e9chelle d’\u00e9l\u00e9ments de la m\u00eame s\u00e9quence isoionique.<\/span><\/p>\n

Mots cl\u00e9s: <\/strong>Ions trivalents de lanthanides, Spectroscopie \u00e0 r\u00e9seau, Approximation du champ central, Alg\u00e8bre de Racah-slater, Erbium, Dysprosium, Holmium, Niveaux d’\u00e9nergie, Longueurs d’onde, Probabilit\u00e9s de transition, configurations \u00e9lectroniques.<\/span><\/p>\n

Abstract<\/strong><\/span><\/p>\n

This thesis focuses on the study of the spectroscopic properties of trivalent rare earth ions, such as Er3+<\/sup>, Dy3+<\/sup>and Ho3+<\/sup>. For the ErIV ion, we analyzed and heard the VUV spectrum in the region ranging from 705 to 2460 \u00c5, and this, using an ab-initio<\/em> method implemented in the RD Cowan code which uses the approximation of the central field and the Racah-slater algebra. Using the experimental spectra recorded with the 10.7m spectrograph from the Paris-Meudon observatory, this made it possible to identify 1022 new lines of transitions between the f11<\/sup>, f10<\/sup>d, f10<\/sup>s, f10<\/sup>p configurations of the ion Er3+<\/sup> added to 591 lines identified previously. These identifications have the effect of determining 168 new energy levels of ErIV for an average deviation of 51cm-1<\/sup>for the configurations of odd parity (f11<\/sup> ~and f10<\/sup>p) and 53 cm-1<\/sup>for the even configurations (f10<\/sup>dand f10<\/sup>s). The large number of experimental levels identified gives a better definition of the Racah parameters, which improves the prediction of the unknown levels and the transitions probabilities.For the Dy3+<\/sup> and the Ho3+<\/sup>, the lack of experimental data compels us to restrict ourselves to purely theoretical calculations adjusted using scale factors of elements of the same isoionic sequence.<\/span><\/p>\n

Keywords: <\/strong>Trivalent lanthanide ions, Grating spectroscopy, Approximation of the central field, Racah-slater algebra, Erbium,\u00a0 Dysprosium, Holmium, Energy levels, Wavelengths, Transitions probabilities, Electronics configurations.<\/span><\/p>\n","protected":false},"excerpt":{"rendered":"

Monsieur CHIKH Anis soutiendra sa th\u00e8se de doctorat 3\u00e8me cycle\u00a0 en physique, intitul\u00e9e: \u00a0Etude des propri\u00e9t\u00e9s radiatives d\u2019ions de terres rares\u00a0: cas des ions Er3+, Dy3+ et Ho3+\u00a0 Date de soutenance: 03 octobre 2021 Lieu de soutenance: Salle de visioconf\u00e9rence du centre des syst\u00e8mes et r\u00e9seaux (Campus Bastos). Jury de soutenance: Nom et Pr\u00e9nom Grade […]<\/p>\n","protected":false},"author":20,"featured_media":6032,"comment_status":"open","ping_status":"open","sticky":false,"template":"","format":"aside","meta":{"_et_pb_use_builder":"","_et_pb_old_content":"","_et_gb_content_width":"","footnotes":""},"categories":[1],"tags":[],"class_list":["post-6017","post","type-post","status-publish","format-aside","has-post-thumbnail","hentry","category-non-classe","post_format-post-format-aside"],"yoast_head":"\nAvis de Soutenance de doctorat en Physique de Anis CHIKH le 03\/10\/2021 - Titre du site % Titre du site<\/title>\n<meta name=\"robots\" content=\"index, follow, max-snippet:-1, max-image-preview:large, max-video-preview:-1\" \/>\n<link rel=\"canonical\" href=\"https:\/\/www.ummto.dz\/fs\/avis-de-soutenance-de-doctorat-de-3eme-cycle-en-physique\/\" \/>\n<meta property=\"og:locale\" content=\"fr_FR\" \/>\n<meta property=\"og:type\" content=\"article\" \/>\n<meta property=\"og:title\" content=\"Avis de Soutenance de doctorat en Physique de Anis CHIKH le 03\/10\/2021 - Titre du site % Titre du site\" \/>\n<meta property=\"og:description\" content=\"Monsieur CHIKH Anis soutiendra sa th\u00e8se de doctorat 3\u00e8me cycle\u00a0 en physique, intitul\u00e9e: \u00a0Etude des propri\u00e9t\u00e9s radiatives d\u2019ions de terres rares\u00a0: cas des ions Er3+, Dy3+ et Ho3+\u00a0 Date de soutenance: 03 octobre 2021 Lieu de soutenance: Salle de visioconf\u00e9rence du centre des syst\u00e8mes et r\u00e9seaux (Campus Bastos). 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