Astronomy and Astrophysics – Astrophysics
Scientific paper
2002-05-10
Astronomy and Astrophysics
Astrophysics
8 pages of text 97 pages of tables submitted to Atomic & Data Nuclear Datables
Scientific paper
10.1016/S0092-640X(03)00056-1
Transition wavelengths and rates are given for E1, E2, M1, and M2 transitions between singlet and triplet S, P, D, and F states in heliumlike ions of astrophysical interest: carbon, nitrogen, oxygen, neon, silicon, and argon. All possible transitions between states with n <= 6 are considered. Wave functions and energies are calculated using the relativistic configuration-interaction (CI) method including both Coulomb and Breit interactions. For transitions to the ground state, the present theoretical wavelengths agree to five digits with precise measurements.
Johnson William R.
Safronova U. I.
Savukov I. M.
No associations
LandOfFree
Multipole (E1, M1, E2, M2) transition wavelengths and rates between states with n<= 6 in heliumlike carbon, nitrogen, oxygen, neon, silicon, and argon does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Multipole (E1, M1, E2, M2) transition wavelengths and rates between states with n<= 6 in heliumlike carbon, nitrogen, oxygen, neon, silicon, and argon, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Multipole (E1, M1, E2, M2) transition wavelengths and rates between states with n<= 6 in heliumlike carbon, nitrogen, oxygen, neon, silicon, and argon will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-497640