L. Abu El Maati, M. Ahmad, I. S. Mahmoud, S. Tawfik, N. Alwadii, N. Ben Nessib, M. Dimitrijević
{"title":"XVIII类碳离子的原子结构和跃迁参数","authors":"L. Abu El Maati, M. Ahmad, I. S. Mahmoud, S. Tawfik, N. Alwadii, N. Ben Nessib, M. Dimitrijević","doi":"10.31577/caosp.2022.52.3.44","DOIUrl":null,"url":null,"abstract":". The atomic and transition parameters of carbon-like ions are sig-nificant for many important astrophysical researches, such as the modeling of stellar atmospheres, the determination of stellar abundance, the analysis of spectral lines for laboratory plasmas or astronomical objects. In this contri-bution, we calculated the energy levels and lifetimes of the carbon-like vanadium ion (V XVIII) using the atomic structure codes AUTOSTRUCTURE and GRASP2018. Weighted oscillator strengths and transition probabilities are also calculated for the allowed transitions between the energy levels considered. The calculations were carried out for the first 17 configurations: 2s 2 2p 2 , 2p 4 , 2s 2 2p3p, 2s2p 2 3s, 2s2p 2 3d, 2p 3 3p, 2s 2 2p4p, 2s 2 3d 2 , 2s2p 3 , 2s 2 2p3s, 2s 2 2p3d, 2s2p 2 3p, 2p 3 3s, 2p 3 3d, 2s 2 2p4s, 2s 2 2p4d and 2s2p3d 2 .","PeriodicalId":50617,"journal":{"name":"Contributions of the Astronomical Observatory Skalnate Pleso","volume":" ","pages":""},"PeriodicalIF":0.4000,"publicationDate":"2022-12-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":"{\"title\":\"Atomic structure and transition parameters of the V XVIII carbon-like ion\",\"authors\":\"L. Abu El Maati, M. Ahmad, I. S. Mahmoud, S. Tawfik, N. Alwadii, N. Ben Nessib, M. Dimitrijević\",\"doi\":\"10.31577/caosp.2022.52.3.44\",\"DOIUrl\":null,\"url\":null,\"abstract\":\". The atomic and transition parameters of carbon-like ions are sig-nificant for many important astrophysical researches, such as the modeling of stellar atmospheres, the determination of stellar abundance, the analysis of spectral lines for laboratory plasmas or astronomical objects. In this contri-bution, we calculated the energy levels and lifetimes of the carbon-like vanadium ion (V XVIII) using the atomic structure codes AUTOSTRUCTURE and GRASP2018. Weighted oscillator strengths and transition probabilities are also calculated for the allowed transitions between the energy levels considered. The calculations were carried out for the first 17 configurations: 2s 2 2p 2 , 2p 4 , 2s 2 2p3p, 2s2p 2 3s, 2s2p 2 3d, 2p 3 3p, 2s 2 2p4p, 2s 2 3d 2 , 2s2p 3 , 2s 2 2p3s, 2s 2 2p3d, 2s2p 2 3p, 2p 3 3s, 2p 3 3d, 2s 2 2p4s, 2s 2 2p4d and 2s2p3d 2 .\",\"PeriodicalId\":50617,\"journal\":{\"name\":\"Contributions of the Astronomical Observatory Skalnate Pleso\",\"volume\":\" \",\"pages\":\"\"},\"PeriodicalIF\":0.4000,\"publicationDate\":\"2022-12-01\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"0\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"Contributions of the Astronomical Observatory Skalnate Pleso\",\"FirstCategoryId\":\"101\",\"ListUrlMain\":\"https://doi.org/10.31577/caosp.2022.52.3.44\",\"RegionNum\":4,\"RegionCategory\":\"物理与天体物理\",\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"Q4\",\"JCRName\":\"ASTRONOMY & ASTROPHYSICS\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"Contributions of the Astronomical Observatory Skalnate Pleso","FirstCategoryId":"101","ListUrlMain":"https://doi.org/10.31577/caosp.2022.52.3.44","RegionNum":4,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q4","JCRName":"ASTRONOMY & ASTROPHYSICS","Score":null,"Total":0}
Atomic structure and transition parameters of the V XVIII carbon-like ion
. The atomic and transition parameters of carbon-like ions are sig-nificant for many important astrophysical researches, such as the modeling of stellar atmospheres, the determination of stellar abundance, the analysis of spectral lines for laboratory plasmas or astronomical objects. In this contri-bution, we calculated the energy levels and lifetimes of the carbon-like vanadium ion (V XVIII) using the atomic structure codes AUTOSTRUCTURE and GRASP2018. Weighted oscillator strengths and transition probabilities are also calculated for the allowed transitions between the energy levels considered. The calculations were carried out for the first 17 configurations: 2s 2 2p 2 , 2p 4 , 2s 2 2p3p, 2s2p 2 3s, 2s2p 2 3d, 2p 3 3p, 2s 2 2p4p, 2s 2 3d 2 , 2s2p 3 , 2s 2 2p3s, 2s 2 2p3d, 2s2p 2 3p, 2p 3 3s, 2p 3 3d, 2s 2 2p4s, 2s 2 2p4d and 2s2p3d 2 .
期刊介绍:
Contributions of the Astronomical Observatory Skalnate Pleso" (CAOSP) is published by the Astronomical Institute of the Slovak Academy of Sciences (SAS). The journal publishes new results of astronomical and astrophysical research, preferentially covering the fields of Interplanetary Matter, Stellar Astrophysics and Solar Physics. We publish regular papers, expert comments and review contributions.