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Published on: December 3, 2013
Hyperfine structure constants for singly-ionized manganese (Mn II) using Fourier Transform Spectroscopy.
Keeley Townley-Smith1, Gillian Nave2, Juliet C Pickering3
1Lamar University, Beaumont, TX 77710, U.S.A.
This study verifies hyperfine magnetic dipole constants (A) for Mn II levels, adding new constants for 47 unstudied levels. Improved accuracy for the ground level constant aids atomic physics research.
Area of Science:
- Atomic Physics
- Spectroscopy
- Quantum Mechanics
Background:
- Building upon the foundational work of Holt et al. (1999) on manganese ion (Mn II) hyperfine structure (HFS).
- Addressing the need for more precise hyperfine magnetic dipole constants (A) in atomic databases.
- Previous measurements by Holt et al. (1999) and Blackwell-Whitehead et al. (2005b) provide a basis for comparison.
Purpose of the Study:
- To expand the understanding of hyperfine structure (HFS) in Mn II.
- To verify existing hyperfine magnetic dipole constants (A) for 20 Mn II energy levels.
- To derive new A constants for 47 previously unstudied Mn II energy levels.
Main Methods:
- Analysis of archival Fourier transform (FT) spectra obtained from Imperial College London and the National Institute of Standards and Technology.
- Utilizing the XGREMLIN software package for the detailed analysis of FT spectra.
- Measurement and calculation of hyperfine magnetic dipole constants (A) from observed HFS patterns.
Main Results:
- Successful verification of hyperfine magnetic dipole constants (A) for 20 previously studied Mn II levels.
- Derivation of A constants for 47 previously unstudied Mn II levels, significantly expanding the available data.
- Achieved a ground level A constant with an uncertainty six times lower than previously reported by Blackwell-Whitehead et al. (2005b).
Conclusions:
- The study successfully expands the knowledge of Mn II hyperfine structure.
- The derived hyperfine magnetic dipole constants (A) offer improved accuracy, particularly for the ground level.
- These findings contribute valuable, high-precision atomic data for astrophysical and fundamental physics applications.
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