On the effective vibrational temperature of the source using (2)3∏ - X3∏ system of GeC molecule

IF 1.9 4区 物理与天体物理 Q2 ASTRONOMY & ASTROPHYSICS
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引用次数: 0

Abstract

In this work, the experimental potential energy curves for (2)3Π and X3Π 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 (2)3ΠX3Π 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 (2)3ΠX3Π 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.

利用 GeC 分子的 (2)3∏ - X3∏ 体系计算源的有效振动温度
本研究采用 Rydberg-Klein-Rees (RKR) 方法构建了 GeC 分子 (2)3Π 和 X3Π 电子态的实验势能曲线。根据 Rydberg-Klein-Rees (RKR) 电位,对实验观测到的 GeC 分子 (2)3Π-X3Π 系统的辐射转变参数,即 Franck-Condon (FC) 因子、r-中心点、电子转变矩、能带强度、相对能带强度、爱因斯坦系数、辐射寿命和振荡器强度进行了估算,并将估算值列表。结果发现 GeC 分子的 (2)3Π-X3Π 系统的有效振动温度为 5628 K。辐射转变参数和有效振动温度表明,太阳和太阳黑子大气中可能存在 GeC 分子。此外,这些参数还可用于天体化学和天体物理观测的合理化。
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来源期刊
Astronomy and Computing
Astronomy and Computing ASTRONOMY & 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.
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