Multiconfiguration Dirac-Fock results for forbidden transitions in the 2p
4 configuration

• Authors: Feng Hu , Jiamin Yang , Chuanke Wang , Gang Jiang , Xuefeng Zhao , Huaping Zang
• Languages of publication: EN

Abstracts

EN

Relativistic configuration interaction calculations with the inclusion of the Breit interaction, quantum electrodynamics and finite nuclear mass corrections have been carried out in the extended optimal level scheme using multiconfiguration Dirac-Fock wavefunctions on the forbidden transition probabilities for the 2p
4 ground state configuration of the oxygen isoelectronic sequence for 8 ⩽ Z ⩽ 42. Electric quadrupole and magnetic dipole transition probabilities are reported for transitions between several of these levels. Our results are compared with those from other theories and experiments. Our energy levels are in better agreement with experiment than other theories.

Keywords

EN

energy level; transition probabilities; multiconfiguration Dirac-Fock; fine structure; life time

• Publisher: De Gruyter Open
• Journal: Open Physics
• Year: 2011
• Volume: 9
• Issue: 5
• Pages: 1228-1236

Dates

published

1 - 10 - 2011

online

15 - 9 - 2011

Contributors

author

Feng Hu

author

Jiamin Yang

• Research Center of Laser Fusion, China Academy of Engineering Physics, Mianyang, 621900, China

author

Chuanke Wang

author

Gang Jiang

• Institute of Atomic and Molecular Physics, Sichuan University, Chengdu, 610064, China

author

Xuefeng Zhao

• Institute of Atomic and Molecular Physics, Sichuan University, Chengdu, 610064, China

author

Huaping Zang

• Institute of Atomic and Molecular Physics, Sichuan University, Chengdu, 610064, China

References

• [1] K.L. Baluja, C.J. Zeippen, J. Phys. B-At. Mol. Opt. 21, 1455 (1988) http://dx.doi.org/10.1088/0953-4075/21/9/007[Crossref]
• [2] B. Edlén, Phys. Scripta 26, 71 (1982) http://dx.doi.org/10.1088/0031-8949/26/2/003[Crossref]
• [3] E. Hinnov, S. Suckewwr, K. Sato, Phys. Rev. A 25, 2293 (1982) http://dx.doi.org/10.1103/PhysRevA.25.2293[Crossref]
• [4] N.J. Peacock, M.F. Stamp, J.D. Silver, Phys. Scripta T8, 10 (1984) http://dx.doi.org/10.1088/0031-8949/1984/T8/002[Crossref]
• [5] W. Eissner, M. Jones, H. Nussbaumer, Comput. Phys. Commun. 8, 270 (1983) http://dx.doi.org/10.1016/0010-4655(74)90019-8[Crossref]
• [6] S.O. Kastner, A.K. Bhatia, L. Cohen, Phys. Scripta 15, 259 (1977) http://dx.doi.org/10.1088/0031-8949/15/4/006[Crossref]
• [7] A.K. Bathia, U. Feldman, G.A. Doschek, Astron. Astrophys. 80, 22 (1979)
• [8] M.E. GalavÍs, C. Mendoza, C.J. Zeippen, Astron. Astrophys. Sup. 123, 159 (1997) http://dx.doi.org/10.1051/aas:1997344[Crossref]
• [9] K.T. Chen, Y.K. Kim, J.P. Desclaux, Atom. Data Nucl. Data 24, 111 (1979) http://dx.doi.org/10.1016/0092-640X(79)90006-8[Crossref]
• [10] B. Edlén, Phys.Scripta 28, 51 (1983) http://dx.doi.org/10.1088/0031-8949/28/1/007[Crossref]
• [11] C.Froese Fischer, H.P. Saha, Phys. Rev. A 28, 3169 (1983) http://dx.doi.org/10.1103/PhysRevA.28.3169[Crossref]
• [12] J.P. Marques, E. Parente, P. Indelicato, Hyperfine Interact. 146–147, 121 (2005)
• [13] E. Landi, Astron. Astrophys. 434, 365 (2005) http://dx.doi.org/10.1051/0004-6361:20042100[Crossref]
• [14] P. Bogdanovich, R. Karuškienė, I. Martinson, Phys. Scripta 67, 44 (2003) http://dx.doi.org/10.1238/Physica.Regular.067a00044[Crossref]
• [15] P. Bogdanovich, D. Majus, T. Pakhomova, Phys. Scripta 74, 558 (2006) http://dx.doi.org/10.1088/0031-8949/74/5/013[Crossref]
• [16] P. Bogdanovich, R. Karuškienė, Atom. Data Nucl. Data 94, 623 (2008) http://dx.doi.org/10.1016/j.adt.2008.01.002[Crossref]
• [17] F. Hu, G. Jiang, W. Hong, L.H. Hao, Eur. Phys. J. D 49, 293 (2008) http://dx.doi.org/10.1140/epjd/e2008-00179-x[Crossref]
• [18] L.H. Hao, G. JIang, S.Q. Song, F. Hu, Atom. Data Nucl. Data 94, 739 (2008) http://dx.doi.org/10.1016/j.adt.2008.05.001[Crossref]
• [19] F.A. Parpia, C.Froese Fischer, I.P. Grant, Comput. Phys. Commun. 94, 249 (1996) http://dx.doi.org/10.1016/0010-4655(95)00136-0[Crossref]
• [20] I.P. Grant, B. J. Mckenzie, P.H. Norrington, D.F. Mayers, N.C. Pyper, Comput. Phys. Commun. 21, 207 (1980) http://dx.doi.org/10.1016/0010-4655(80)90041-7[Crossref]
• [21] I. Kinek, L. Engström, U. Feldman, Astrophys. J 512, 496 (1996) http://dx.doi.org/10.1086/306738[Crossref]
• [22] A. Omholt, The airglow and the aurore (Pergamon, London, 1956)
• [23] S. Chung, L.C. Chun, C. FroeseFischer, L. P. T. Edward, J. Chem. Phys. 76, 498 (1982) http://dx.doi.org/10.1063/1.442751[Crossref]
• [24] C. Nicolaides, O. Sinanoǧlu, P. Westhaus, Phys. Rev. A4, 1400 (1971)
• [25] R.H. Garstang, Mon. Not. R. Astron. Soc 111, 115 (1951)
• [26] F.J. LeBlanc, O. Oldenberg, N.P. Carleton, J. Chem. Phys. 45, 2200 (1966) http://dx.doi.org/10.1063/1.1727909[Crossref]
• [27] J.W. McConkey, D.J. Burns, K.A. Moran, K.G. Emeleus, Phys. Lett. 22, 416 (1966) http://dx.doi.org/10.1016/0031-9163(66)91206-6[Crossref]
• [28] J.A. Kernahan, P.H-L Pang, Can. J. Phys. 53, 455 (1975) http://dx.doi.org/10.1139/p75-058[Crossref]
• [29] A. Corney, O.M. Williams, J. Phys. B-At. Mol. Opt. 5, 686 (1972) http://dx.doi.org/10.1088/0022-3700/5/3/035[Crossref]
• [30] W.F.J. Evans, A. Vallance Jones, Can. J. Phys. 43, 697 (1965) http://dx.doi.org/10.1139/p65-065[Crossref]

Identifiers

DOI

10.2478/s11534-011-0022-7