Abstract.
Relative transition probabilities for 18 lines of Zn II (11 measured for the first time) were determined from the emission-line intensities in a laser-produced plasma. The experiment was carried out using Cd–Zn alloy with a Zn content under 10% in order to obtain optically thin plasma. Oscillator strengths were placed on an absolute scale by using experimental lifetimes, line-strength sum rules and Boltzmann plot. A comparison has been conducted between present experimental results, the data available and new calculations reported in this work, as well as a study of the plasma conditions.
Similar content being viewed by others
References
S.R. Baumann, W.H. Smith, J. Opt. Soc. Am 60, 345 (1970)
T. Andersen, G. Sørensen, J. Quant. Spectrosc. Radiat. Transfer 13, 369 (1973)
I. Martinson et al., Phys. Scripta 19, 17 (1979)
S. Hultberg, L. Liljeby, A. Lindgård, S. Mannervik, E. Veje, Phys. Scripta 22, 623 (1981)
T. Andersen, O. Poulsen, P.S. Ramanujam, J. Quant. Spectrosc. Radiat. Transfer 16, 521 (1976)
S.D. Bergeson, J.E. Lawler, Astrophys. J. 408, 382 (1993)
NIST – Atomic Spectra Data Base Lines (wavelength order) — http://physics.nist.gov/cgi-bin/AtData/ main-asd (2003)
A. Lindgård, L.J. Curtis, I. Martinson, S.E. Nielsen, Phys. Scripta 21, 47 (1980)
J. Migdalek, W.E. Baylis, J. Phys. B 12, 1113 (1979)
O. Zatsarinny, L. Bandurina, J. Phys. B 32, 4793 (1999)
L.J. Curtis, C.E. Theodosiou, Phys. Rev. A 39, 605 (1989)
C. Laughlin, Z. Phys. D 39, 201 (1997)
B.N. Chichkov, V.P. Shevelko, Phys. Scripta 23, 1055 (1981)
S. Djeniže, V. Milosavljević, M.S. Dimitrijević, Eur. Phys. J. D 27, 209 (2003)
E. Biémont, P.H. Lefèbvre, P. Quinet, S. Svanberg, H.L. Xu, Eur. Phys. J. D 27, 33 (2003)
R. Mayo, M. Ortiz, J. Campos, J. Quant. Spectrosc. Radiat. Transfer 94, 109 (2005)
E. Danezis, E. Theodossiou, Astrophys. J. Suppl. Ser. 174, 49 (1990)
D.A. Verner, P.D. Barthel, D. Tytler, Astron. Astrophys. Suppl. Ser. 108, 287 (1994)
M. Pettini, D.L. King, L.J. Smith, R.W. Hunstead, Astrophys. J. 478, 536 (1997)
M. Pettini, L.J. Smith, D.L. King, R.W. Hunstead, Astrophys. J. 486, 665 (1997)
L.Č. Popović, I. Vince, M.S. Dimitrijević, Astron. Astrophys. Suppl. Ser. 102, 17 (1993)
K.C. Smith, Astron. Astrophys. 291, 521 (1994)
B.D. Savage, J.A. Cardelli, U.J. Sofia, Astrophys. J. 401, 706 (1992)
M. Gemišić Adamov, M.M. Kuraica, N. Konjević, Eur. Phys. J. D 28, 393 (2004)
S.A. Harrison, A. Hibbert, Mon. Not. R. Astron. Soc. 340, 1279 (2003)
K.B. Blagoev et al., Phys. Scripta 69, 433 (2004)
J. Sugar, A. Musgrove, J. Phys. Chem. Ref. Data 24 6, 1803 (1995)
D. Gullberg, U. Litzén, Phys. Scripta 61, 652 (2000)
R.D. Cowan, The Theory of Atomic Structure and Spectra (Berkeley U. California Press, Los Angeles, 1981)
A.P. Thorne, Spectrophysics (Chapman and Hall, London, 1988)
H.S. Chou, W.R. Johnson, Phys. Rev. A 56 3, 2424 (1997)
S.G. Nana Engo et al., Phys. Rev. A 56 4, 2624 (1997)
G. Lagmago Kamta, S.G. Nana Engo, M.G. Kwato Njock, B. Oumarou, J. Phys. B 31, 963 (1998)
Author information
Authors and Affiliations
Corresponding author
Rights and permissions
About this article
Cite this article
Mayo, R., Ortiz, M. & Campos, J. Experimental oscillator strengths of Zn II lines of astrophysical interest. Eur. Phys. J. D 37, 181–186 (2006). https://doi.org/10.1140/epjd/e2005-00283-5
Received:
Published:
Issue Date:
DOI: https://doi.org/10.1140/epjd/e2005-00283-5