2004
DOI: 10.1063/1.1687725
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Prospects for high-gain, high yield National Ignition Facility targets driven by 2ω (green) light

Abstract: The National Ignition Facility (NIF) [J. A. Paisner, E. M. Campbell, and W. J. Hogan, Fusion Technol. 26, 755 (1994)], operating at green (2ω) light, has the potential to drive ignition targets with significantly more energy than the 1.8 MJ it will produce with its baseline, blue (3ω) operations. This results in a greatly increased “target design space,” providing a number of exciting opportunities for fusion research. These include the prospect of ignition experiments with capsules absorbing energies in the v… Show more

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Cited by 30 publications
(23 citation statements)
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“…Thus, post ignition pressures and temperatures are very different from pre-ignition numbers. Larger ICF capsules that are designed for high-gain fusion experiments [79,80] use about an order of magnitude more fuel, but overall the P τ conditions are not be very different.…”
Section: Pressurementioning
confidence: 99%
“…Thus, post ignition pressures and temperatures are very different from pre-ignition numbers. Larger ICF capsules that are designed for high-gain fusion experiments [79,80] use about an order of magnitude more fuel, but overall the P τ conditions are not be very different.…”
Section: Pressurementioning
confidence: 99%
“…The two issues greatly limit the maximum energy output capability of a 3ω laser facility. In contrast, 2ω laser can highly increase the threshold for optical damages, which therefore results in a lower operation costs for a laser facility and a higher laser energy deliverable on target [11,12]. Furthermore, in the long term, any reactor based on laser-driven ICF will require laser operation at sufficiently high wavelength for keeping the live time of the optics at a level that meets the energy production requirements [13].…”
Section: Introductionmentioning
confidence: 99%
“…34 It may also be possible to study thermonuclear reactions in highly screened, dense plasmas, relevant to reactions in dwarf stars. Finally, if high gain ͑G Ͼ 100͒ implosions can be produced, 35 it may be possible to examine some of the physics issues surrounding the proposed deflagration-to-detonation transition, and the role of hydrodynamic mixing, relevant to type la supermovas. 36 …”
Section: A Burning Plasmasmentioning
confidence: 99%