K-shell spectra from hot dense aluminum layers buried in carbon and heated by ultrashort laser pulses

被引:54
作者
Eidmann, K [1 ]
Andiel, U
Pisani, F
Hakel, P
Mancini, RC
Junkel-Vives, GC
Abdallah, J
Witte, K
机构
[1] Max Planck Inst Quantum Opt, D-85748 Garching, Germany
[2] Univ Nevada, Dept Phys, Reno, NV 89557 USA
[3] Los Alamos Natl Lab, Los Alamos, NM 87545 USA
关键词
K-shell spectroscopy; short pulse laser; spectral line shifts;
D O I
10.1016/S0022-4073(03)00067-0
中图分类号
O43 [光学];
学科分类号
070207 ; 0803 ;
摘要
Ultrashort laser pulses allow for the generation of hot plasmas near solid state densities. For this purpose a Ti:Sapphire laser was used, which delivers after frequency doubling, pulses of high contrast with an energy of about 60 mJ and a duration of 150 fs at 395 run. The typical intensity on the target was a few 10(17) W/cm(2). To achieve a high degree of uniformity we used targets consisting of a 25 run thin Al tracer layer buried at different depths up to 400 nm in solid carbon. Time-integrated Al K-shell spectra are presented. Characteristic features of the spectra are significant high-order satellite line emission, strong line broadening and a center-of-mass line shift to the red, which was observed in transitions from principal quantum number n = 2 or 3 to 1. Accurate measurement of the shift was made possible by using the cold Si K-alpha line as an absolute wavelength calibration. In addition to time-integrated measurements, we used an ultrafast X-ray streak camera to obtain time and spectrally resolved spectra. Typical durations of the Ly(alpha) and He-alpha lines are in the range 2-4 ps. The experimental results are compared with a time-dependent model, which combines hydrodynamic simulations, time-dependent atomic kinetics, detailed spectral line shapes including line shifts, and radiation transport. (C) 2003 Elsevier Science Ltd. All rights reserved.
引用
收藏
页码:133 / 146
页数:14
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