Lifetime of a K-shell vacancy in atomic carbon created by 1s→2p photoexcitation of C+

被引:53
作者
Schlachter, AS
Sant'Anna, MM
Covington, AM
Aguilar, A
Gharaibeh, MF
Emmons, ED
Scully, SWJ
Phaneuf, RA
Hinojosa, G
Alvarez, I
Cisneros, C
Müller, A
McLaughlin, BM
机构
[1] Univ Calif Berkeley, Lawrence Berkeley Lab, Adv Light Source, Berkeley, CA 94720 USA
[2] Harvard Smithsonian Ctr Astrophys, Inst Theoret Atom & Mol Phys, Cambridge, MA 02138 USA
[3] Univ Giessen, Inst Kernphys, D-35392 Giessen, Germany
[4] Univ Nacl Autonoma Mexico, Ctr Ciencias Fis, Cuernavaca 62131, Morelos, Mexico
[5] Univ Nevada, Dept Phys, Reno, NV 89557 USA
[6] Lake Tahoe Community Coll, Dept Phys, S Lake Tahoe, CA 96150 USA
关键词
D O I
10.1088/0953-4075/37/5/L03
中图分类号
O43 [光学];
学科分类号
070207 ; 0803 ;
摘要
Lifetimes for K-shell vacancy states in atomic carbon have been determined by measurement of the natural linewidth of the 1s --> 2p photoexcited states of C+ ions. The K-shell vacancy states produced by photoionization of atomic carbon are identical to those produced by 1s --> 2p photoexcitation of a C+ ion: 1s2S(2) 2p(2) D-2, P-2, and S-2 autoionizing states occur in both cases. These vacancy states stabilize by emission of an electron to produce C2+ ions. Measurements are reported for the lifetime of the 1s2s(2) 2p(2) D-2, P-2 and S-2 autoionizing states of C+: 6.3 +/- 0.9 fs, 11.2 +/- 1.1 fs and 5.9 +/- 1.3 fs respectively. Knowledge of such lifetimes is important for comparative studies of the lifetimes of K-shell vacancies in carbon-containing molecules, benchmarking theory, and interpreting satellite x-ray spectra from astrophysical sources such as x-ray binaries. Absolute cross sections were measured for both ground-state and metastable-state ions providing a stringent test of state-of-the-art theoretical calculations.
引用
收藏
页码:L103 / L109
页数:7
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