Lα X-ray satellites for 31 ≤ Z ≤ 38: Systematization
Desh Deepak Tewari1, Garima Misra2, U.D.Misra3
1Desh Deepak Tewari, Department of Applied Sciences, Institute of Engineering and Technology, Lucknow, U.P., India.
2Garima Misra, Department of Applied Sciences, Shri Ramswaroop memorial college of Engineering and Management, Lucknow, U.P., India.
3U.D.Misra*, Physics Department, Lucknow University, Lucknow, U.P., India.
Manuscript received on November 12, 2019. | Revised Manuscript received on November 25, 2019. | Manuscript published on 30 November, 2019. | PP: 5275-5278 | Volume-8 Issue-4, November 2019. | Retrieval Number: D7450118419/2019©BEIESP | DOI: 10.35940/ijrte.D7450.118419
Open Access | Ethics and Policies | Cite | Mendeley | Indexing and Abstracting
© The Authors. Blue Eyes Intelligence Engineering and Sciences Publication (BEIESP). This is an open access article under the CC-BY-NC-ND license (http://creativecommons.org/licenses/by-nc-nd/4.0/)
Abstract: An examination of the problem of the energy values, their interpretation and the origin of the Lα x – ray satellites in the atomic number range Z = 31-38 reveals non existence and lack of sufficient data for the purpose. The energies of these satellites where not available are obtained using suitable semi-empirical method for the elements under investigation and the available systematization procedures namely Mosley plot and the self consistent doubly modified Mosley plot are considered. It is concluded that the self consistent method is not applicable in the present scenario. The energy values for the satellites Lα5, Lα6 and Lα7 are calculated using Mosley plot for the atomic number range Z= 31 to 35 and are reported for the first time.
Keywords: Lα Satellites, Systematization, Mosley Plot, Spectator Vacancy, Transitions.
Scope of the Article: Multi-Agent Systems.