Electric Dipole Transition Parameters for 5s-5p and 5p-5d Transitions in Doubly Ionized Xenon

• Authors: S. Eser , L. Özdemir
• Languages of publication: EN

Abstracts

EN

Using the general-purpose relativistic atomic structure package based on the fully relativistic multiconfiguration Dirac-Fock method, we have reported the electric dipole transition (E1) parameters such as wavelengths, weighted oscillator strengths, transition rates (or probabilities) and line strengths for 5s-5p and 5p-5d transitions in Xe²⁺. In calculations, the Breit interaction and quantum electrodynamic effects have been included as perturbations. The calculated values for energy levels including valence and core-valence correlation have been compared with other available experimental and theoretical values in literature. Our transition results can provide useful data for, in particular, experimental works in future.

Keywords

EN

31.15.ag; 32.70.Cs; 31.15.aj; 31.30.-i; 31.15.V-

Discipline

• 31.30.-i: Corrections to electronic structure(see also 03.30.+p Special relativity; for exotic atoms and molecules, see 36.10.-k; for applications of density-functional theory, see 31.15.es)
• 31.15.V-: Electron correlation calculations for atoms, ions and molecules
• 31.15.aj: Relativistic corrections, spin-orbit effects, fine structure; hyperfine structure
• 32.70.Cs: Oscillator strengths, lifetimes, transition moments
• 31.15.ag: Excitation energies and lifetimes; oscillator strengths

• Publisher: Institute of Physics, Polish Academy of Sciences
• Journal: Acta Physica Polonica A
• Year: 2017
• Volume: 132
• Issue: 4
• Pages: 1284-1289

Dates

published

2017-10

received

2016-09-27

(unknown)

2017-04-04

Contributors

author

S. Eser

• Department of Physics, Sakarya University, 54187, Sakarya, Turkey

author

L. Özdemir

• Department of Physics, Sakarya University, 54187, Sakarya, Turkey

References

• [1] S. Fritzsche, A.N. Grum-Grzhimailo, E.V. Gryzlova, N.M. Kabachnik, J. Phys. B At. Mol. Opt. Phys. 44, 175602 (2011), doi: 10.1088/0953-4075/44/17/175602
• [2] E. Träbert, Phys. Scr. 85, 048101 (2012), doi: 10.1088/0031-8949/85/04/048101
• [3] R.J. Peláez, M. Ćirišan, S. Djurović, J.A. Aparicio, S. Mar, J. Phys. B At. Mol. Opt. Phys. 39, 5013 (2006), doi: 10.1088/0953-4075/39/23/017
• [4] J. Reyna Almandos, F. Bredice, M. Raineri, M. Gallardo, Phys. Scr. T 134, 014018 (2009), doi: 10.1088/0031-8949/2009/T134/014018
• [5] R.A. Walch, R.D. Knight, Phys. Rev. A 38, 2375 (1988), doi: 10.1103/PhysRevA.38.2375
• [6] A.G. Calamai, C.E. Johnson, Phys. Rev. A 45, 7792 (1992), doi: 10.1103/PhysRevA.45.7792
• [7] K.G. Bhushan, H.B. Pedersen, N. Altstein, O. Heber, M.L. Rappaport, D. Zajfman, Phys. Rev. A 62, 012504 (2000), doi: 10.1103/PhysRevA.62.012504
• [8] J.E. Hansen, W. Persson, Phys. Scr. 25, 487 (1982), doi: 10.1088/0031-8949/25/3/010
• [9] R.H. Garstang, J. Res. Natl. Bur. Stand. Sec. A 68, 61 (1964), doi: 10.6028/jres.068A.004
• [10] S. Schippers, S. Ricz, T. Buhr, A. Borovik Jr, J. Hellhund, K. Holste, K. Huber, H.-J. Schäfer, D. Schury, S. Klumpp, K. Mertens, M. Martins, R. Flesch, G. Ulrich, E. Rühl, T. Jahnke, J. Lower, D. Metz, L.P.H. Schmidt, M. Schöffler, J.B. Williams, L. Glaser, F. Scholz, J. Seltmann, J. Viefhaus, A. Dorn, A. Wolf, J. Ullrich, A. Müller, J. Phys. B At. Mol. Opt. Phys. 47, 115602 (2014), doi: 10.1088/0953-4075/47/11/115602
• [11] E.B. Saloman, J. Phys. Chem. Ref. Data 33, 765 (2004), doi: 10.1063/1.1649348
• [12] P. Andersen, T. Andersen, F. Folkmann, V.K. Ivanov, H. Kjeldsen, J.B. West, J. Phys. B At. Mol. Opt. Phys. 34, 2009 (2001), doi: 10.1088/0953-4075/34/10/314
• [13] W. Persson, C.G. Wahlström, Phys. Scr. 38, 347 (1988), doi: 10.1088/0031-8949/38/3/005
• [14] V.A. Dzuba, V.V. Flambaum, Phys. Rev. A 75, 052504 (2007), doi: 10.1103/PhysRevA.75.052504
• [15] H. Sobral, M. Raineri, D. Schinca, M. Gallardo, R. Duchowicz, IEEE J. Quantum Electron. 35, 1308 (1999), doi: 10.1109/3.784590
• [16] D.E. Osterbrock, Astrophys. J. 114, 469 (1951), doi: 10.1086/145487
• [17] M. Gallardo, C.A. Massonet, A.A. Tagliaferri, M. Garavaglia, Phys. Scr. 19, 538 (1979), doi: 10.1088/0031-8949/19/5-6/008
• [18] P. Bolognesi, S.J. Cavanagh, L. Avaldi, R. Camilloni, M. Zitnik, M. Stuhec, G.C. King, J. Phys. B At. Mol. Opt. Phys. 33, 4723 (2000), doi: 10.1088/0953-4075/33/21/316
• [19] M. Pernpointner, J. Phys. B At. Mol. Opt. Phys. 43, 205102 (2010), doi: 10.1088/0953-4075/43/20/205102
• [20] K.G. Dyall, I.P. Grant, C.T. Johnson, F.A. Parpia, E.P. Plummer, Comp. Phys. Commun. 55, 425 (1989), doi: 10.1016/0010-4655(89)90136-7
• [21] A. Kramida, Yu. Ralchenko, J. Reader, and NIST ASD Team (2015), NIST Atomic Spectra Database, ver. 5.3, National Institute of Standards and Technology, Gaithersburg (MD) 2016 http://www.nist.gov/pml/atomic-spectra-database

Identifiers

DOI

10.12693/APhysPolA.132.1284