Theoretical L-shell Coster-Kronig energies 11< or =Z< or =103
Relativistic relaxed-orbital calculations of L-shell Coster-Kronig transition energies have been performed ab initio for all possible transitions in atoms with atomic numbers 11 < or =Z< or =103. Hartree-Fock-Slater wavefunctions served as zeroth-order eigenfunctions to compute the expectation of the total Hamiltonian. A first-order approximation to the local approximation was thus included. Quantum-electrodynamic corrections were made. Each transition energy was computed as the difference between results of separate self-consistent-field calculations for the initial, singly ionized state and the final two-hole state. The following quantities are listed: total transition energy, ''electric'' (Dirac-Hartree-Fock-Slater) contribution, magnetic and retardation contributions, and contributions due to vacuum polarization and self energy.
- Research Organization:
- Department of Physics, University of Oregon Eugene, Oregon 97403
- OSTI ID:
- 7319352
- Journal Information:
- At. Data Nucl. Data Tables; (United States), Journal Name: At. Data Nucl. Data Tables; (United States) Vol. 19:2; ISSN ADNDA
- Country of Publication:
- United States
- Language:
- English
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Related Subjects
Molecular & Chemical Physics-- Atomic & Molecular Properties & Theory
74 ATOMIC AND MOLECULAR PHYSICS
ATOMS
AUGER EFFECT
COSTER-KRONIG TRANSITIONS
ENERGY
ENERGY-LEVEL TRANSITIONS
FUNCTIONS
HAMILTONIANS
HARTREE-FOCK METHOD
MATHEMATICAL OPERATORS
QUANTUM OPERATORS
SELF-ENERGY
SLATER METHOD
VACUUM POLARIZATION
WAVE FUNCTIONS