Radiative shocks produced from spherical cryogenic implosions at the National Ignition Facility

Radiative shocks produced from spherical cryogenic implosions at the National Ignition Facility
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DOI:
10.1063/1.4805081
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发表时间:
2013-05
期刊:
影响因子:
2.2
通讯作者:
A. Pak;L. Divol;G. Gregori;S. Weber;J. Atherton;R. Bennedetti;D. Bradley;D. Callahan;D. Casey;E. Dewald;T. Döppner;M. Edwards;J. Frenje;S. Glenn;G. Grim;D. Hicks;W. Hsing;N. Izumi;O. Jones;Maria Gatu Johnson;S. Khan;J. Kilkenny;J. Kline;G. Kyrala;J. Lindl;O. Landen;S. L. Pape;T. Ma;A. MacPhee;B. MacGowan;A. Mackinnon;L. Masse;N. Meezan;J. Moody;R. Olson;J. Ralph;H. Robey;H. Park;B. Remington;J. Ross;R. Tommasini;R. Town;V. Smalyuk;S. Glenzer;E. Moses
A. Pak;L. Divol;G. Gregori;S. Weber;J. Atherton;R. Bennedetti;D. Bradley;D. Callahan;D. Casey;E. Dewald;T. Döppner;M. Edwards;J. Frenje;S. Glenn;G. Grim;D. Hicks;W. Hsing;N. Izumi;O. Jones;Maria Gatu Johnson;S. Khan;J. Kilkenny;J. Kline;G. Kyrala;J. Lindl;O. Landen;S. L. Pape;T. Ma;A. MacPhee;B. MacGowan;A. Mackinnon;L. Masse;N. Meezan;J. Moody;R. Olson;J. Ralph;H. Robey;H. Park;B. Remington;J. Ross;R. Tommasini;R. Town;V. Smalyuk;S. Glenzer;E. Moses
中科院分区:
物理与天体物理3区
文献类型:
--
作者:
A. Pak;L. Divol;G. Gregori;S. Weber;J. Atherton;R. Bennedetti;D. Bradley;D. Callahan;D. Casey;E. Dewald;T. Döppner;M. Edwards;J. Frenje;S. Glenn;G. Grim;D. Hicks;W. Hsing;N. Izumi;O. Jones;Maria Gatu Johnson;S. Khan;J. Kilkenny;J. Kline;G. Kyrala;J. Lindl;O. Landen;S. L. Pape;T. Ma;A. MacPhee;B. MacGowan;A. Mackinnon;L. Masse;N. Meezan;J. Moody;R. Olson;J. Ralph;H. Robey;H. Park;B. Remington;J. Ross;R. Tommasini;R. Town;V. Smalyuk;S. Glenzer;E. Moses

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Spherically expanding radiative shock waves have been observed from inertially confined implosion experiments at the National Ignition Facility. In these experiments, a spherical fusion target, initially 2 mm in diameter, is compressed via the pressure induced from the ablation of the outer target surface. At the peak compression of the capsule, x-ray and nuclear diagnostics indicate the formation of a central core, with a radius and ion temperature of ∼20 μm and ∼ 2 keV, respectively. This central core is surrounded by a cooler compressed shell of deuterium-tritium fuel that has an outer radius of ∼40 μm and a density of >500 g/cm3. Using inputs from multiple diagnostics, the peak pressure of the compressed core has been inferred to be of order 100 Gbar for the implosions discussed here. The shock front, initially located at the interface between the high pressure compressed fuel shell and surrounding in-falling low pressure ablator plasma, begins to propagate outwards after peak compression has been rea...