Photoexcitation of K-shell and L-shell Hollow Beryllium
Creators
- 1. Department of Quantum Engineering and Systems Science, University of Tokyo, Tokyo 113-8656 (Japan)
- 2. School of Medicine, Kitasato University, Kanagawa 228-8555 (Japan)
- 3. Physics Department, Kassel University, D-34132 Kassel (Germany)
- 4. Photon Factory, KEK, Ibaraki 305-0801 (Japan)
- 5. Department of Physics, Meisei University, Tokyo 191-8506 (Japan)
Description
We have observed K-shell and L-shell hollow beryllium atoms (2s22p3s and 1s3s23p) created by photoexcitation using synchrotron radiation. Resonance shapes were fitted to the Fano profile and the parameters were deduced. A Dirac-Fock calculation was performed to identify the configuration of the peaks and to predict other hollow atomic peaks. The results of the calculation were in good agreement with the experimental data. The comparison of the transition strength has revealed that the three-electron photoexcitation to the 1s3s23p configuration is stronger than the two-electron photoexcitation to the 2s22p3s configuration. This is attributed to the large overlap between the 2s orbital of the ground state (1s22s2) with the 3s orbital of the L-shell hollow state (1s3s23p)
Additional details
Identifiers
Publishing Information
- Journal Title
- Physical Review Letters
- Journal Volume
- 97
- Journal Issue
- 2
- Journal Page Range
- p. 023001-023001.4
- ISSN
- 0031-9007
- CODEN
- PRLTAO
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 38023469
- Subject category
- S74: ATOMIC AND MOLECULAR PHYSICS;
- Resource subtype / Literary indicator
- Numerical Data
- Descriptors DEI
- BERYLLIUM; ELECTRONS; EXPERIMENTAL DATA; GROUND STATES; K SHELL; L SHELL; SYNCHROTRON RADIATION
- Descriptors DEC
- ALKALINE EARTH METALS; BREMSSTRAHLUNG; DATA; ELECTROMAGNETIC RADIATION; ELECTRONIC STRUCTURE; ELEMENTARY PARTICLES; ELEMENTS; ENERGY LEVELS; FERMIONS; INFORMATION; LEPTONS; METALS; NUMERICAL DATA; RADIATIONS
Optional Information
- Notes
- (c) 2006 The American Physical Society