{"title":"On the effective vibrational temperature of the source using (2)3∏ - X3∏ system of GeC molecule","authors":"R. Sindhan , N. Venkatesh Bharathi , S. Ramaswamy","doi":"10.1016/j.ascom.2024.100859","DOIUrl":null,"url":null,"abstract":"<div><p>In this work, the experimental potential energy curves for <span><math><mrow><msup><mrow><mo>(</mo><mn>2</mn><mo>)</mo></mrow><mn>3</mn></msup><mstyle><mi>Π</mi></mstyle></mrow></math></span> and <span><math><mrow><msup><mrow><mi>X</mi></mrow><mn>3</mn></msup><mstyle><mi>Π</mi></mstyle></mrow></math></span> electronic states of GeC molecule have been constructed by using Rydberg-Klein-Rees (RKR) method. The radiative transition parameters viz., Franck-Condon (FC) factor, r-centroid, electronic transition moment, band strength, relative band strength, Einstein coefficients, radiative lifetime and oscillator strength for the <span><math><mrow><msup><mrow><mo>(</mo><mn>2</mn><mo>)</mo></mrow><mn>3</mn></msup><mstyle><mi>Π</mi></mstyle><mo>−</mo><msup><mrow><mi>X</mi></mrow><mn>3</mn></msup><mstyle><mi>Π</mi></mstyle></mrow></math></span> system of GeC molecule have been estimated for the experimentally observed vibrational levels from Rydberg-Klein-Rees (RKR) potential and the estimated values are tabulated. The estimated effective vibrational temperature found as 5628 K for the <span><math><mrow><msup><mrow><mo>(</mo><mn>2</mn><mo>)</mo></mrow><mn>3</mn></msup><mstyle><mi>Π</mi></mstyle><mo>−</mo><msup><mrow><mi>X</mi></mrow><mn>3</mn></msup><mstyle><mi>Π</mi></mstyle></mrow></math></span> system of GeC molecule. The radiative transition parameters and effective vibrational temperature are evident that the possible presence of GeC molecule in solar and sunspots atmosphere. Further, these parameters are employed in rationalizations of astrochemical and astrophysical observations.</p></div>","PeriodicalId":48757,"journal":{"name":"Astronomy and Computing","volume":"48 ","pages":"Article 100859"},"PeriodicalIF":1.9000,"publicationDate":"2024-07-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Astronomy and Computing","FirstCategoryId":"101","ListUrlMain":"https://www.sciencedirect.com/science/article/pii/S221313372400074X","RegionNum":4,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q2","JCRName":"ASTRONOMY & ASTROPHYSICS","Score":null,"Total":0}
引用次数: 0
Abstract
In this work, the experimental potential energy curves for and electronic states of GeC molecule have been constructed by using Rydberg-Klein-Rees (RKR) method. The radiative transition parameters viz., Franck-Condon (FC) factor, r-centroid, electronic transition moment, band strength, relative band strength, Einstein coefficients, radiative lifetime and oscillator strength for the system of GeC molecule have been estimated for the experimentally observed vibrational levels from Rydberg-Klein-Rees (RKR) potential and the estimated values are tabulated. The estimated effective vibrational temperature found as 5628 K for the system of GeC molecule. The radiative transition parameters and effective vibrational temperature are evident that the possible presence of GeC molecule in solar and sunspots atmosphere. Further, these parameters are employed in rationalizations of astrochemical and astrophysical observations.
Astronomy and ComputingASTRONOMY & ASTROPHYSICSCOMPUTER SCIENCE,-COMPUTER SCIENCE, INTERDISCIPLINARY APPLICATIONS
CiteScore
4.10
自引率
8.00%
发文量
67
期刊介绍:
Astronomy and Computing is a peer-reviewed journal that focuses on the broad area between astronomy, computer science and information technology. The journal aims to publish the work of scientists and (software) engineers in all aspects of astronomical computing, including the collection, analysis, reduction, visualisation, preservation and dissemination of data, and the development of astronomical software and simulations. The journal covers applications for academic computer science techniques to astronomy, as well as novel applications of information technologies within astronomy.