2011
DOI: 10.1016/j.hedp.2011.05.011
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Spectroscopic observations of Fermi-degenerate aluminum compressed and heated to four times solid density and 20 eV

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Cited by 5 publications
(5 citation statements)
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“…Aluminum, a simple metal, has been one of the most commonly-studied prototype materials for gaining insight into physical properties at such conditions. The wide breadth of experimental and theoretical research on aluminum includes studies of solid phase transitions [6,7], shock physics [8][9][10][11][12][13][14][15][16][17][18], x-ray diagnostics for basic plasma physics [19][20][21][22][23][24][25][26][27][28][29][30][31][32][33][34], and optical [35][36][37][38][39] and transport [40][41][42][43][44][45][46][47] properties.…”
Section: Introductionmentioning
confidence: 99%
“…Aluminum, a simple metal, has been one of the most commonly-studied prototype materials for gaining insight into physical properties at such conditions. The wide breadth of experimental and theoretical research on aluminum includes studies of solid phase transitions [6,7], shock physics [8][9][10][11][12][13][14][15][16][17][18], x-ray diagnostics for basic plasma physics [19][20][21][22][23][24][25][26][27][28][29][30][31][32][33][34], and optical [35][36][37][38][39] and transport [40][41][42][43][44][45][46][47] properties.…”
Section: Introductionmentioning
confidence: 99%
“…This is the first observation of plasma conditions created with a compression wave. 24 The level of shock-wave heating and timing of heat-front penetration inferred from the experiments were compared with the post-processed LILAC simulations using the time-dependent atomic physics code Spect3D. 25 The shock-wave heating and heat-front penetration predicted by LILAC using f = 0.06 or the nonlocal model agree with experimental results for times when the shock is transiting the foil.…”
Section: T Tmentioning
confidence: 90%
“…This is the first measurement of the plasma temperature and density in a direct-drive target created by multiple shock waves (i.e., a weak shock and a compression wave). 24 The best fit to each spectrum is represented by the black curve. The mass densities inferred are between 5 and 7 g/cm 3 for the 1-ns square laser pulse [ Fig.…”
Section: Draco (2-d)mentioning
confidence: 99%
See 1 more Smart Citation
“…Significant advances made in inertial confinement fusion (ICF) research have been enabled by x-ray spectroscopy, thus contributing to a better interpretation of the underlying physics and target performance, and to improvements in the predictive capability of simulation codes [1,2]. Among these achievements are: the measurement of target preheat due to fast electrons by means of Kα emission spectroscopy [3][4][5]; the extraction of spatially averaged electron temperature and density in implosion cores of direct-and indirect-drive implosions by analyzing Starkbroadened K-and L-shell line emissions [6][7][8][9][10][11][12][13][14]; the use of K-shell absorption spectroscopy to infer the conditions of the relatively cold imploding shell that confines the core [15][16][17][18][19]; the simultaneous determination of time-and space-averaged conditions for both core and shell in thick-wall targets by accounting for the attenuation of core x-ray emission in the compressed shell [20]; the time-resolved characterization and energy balance analysis of implosion core in shock-ignition experiments [21]; the quantitative evaluation of mixing of ablator material into the hot-spot of ignition-scale targets from the K-shell emission of mid-Z dopant elements [22][23][24]; the extraction of spatial profiles of temperature and density from the analysis of x-ray spectra and narrow-band images [25][26][27]; the asymmetry measurement of plasma temperature and density spatial profiles from pinhole space-resolved spectra [28]; and the observation of three-dimensional and laser imprinting effects in polar-drive implosions with gated spectrally resolved x-ray imaging [29]. Furthermore, the conditions achieved in laser-driven ICF capsules are similar to those in stellar interior environments, so this progress in ICF research is also likely to benefit applications in astrophysics [30].…”
Section: Introductionmentioning
confidence: 99%