Abstract
The origin of the fine structure in the wings of the broadened atomic resonance lines of rare gases is discussed. A theoretical model is developed, which enables to ascertain the contributions to absorption by free and bound pairs of rare gas atoms. The quantum-mechanical approach with vibrational-rotational interaction taken into account is employed for bound pairs, and binary quasistatic approximation is used for free pairs. The theory is applied to the computation of the absorption profiles related to the low-energy tail of the first resonance line (1469.60 Å) of gaseous xenon.
Sign-in/Register to access full text options 
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Schedule a callDisclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.
