2012
DOI: 10.1063/1.4737157
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Burning plasmas with ultrashort soft-x-ray flashing

Abstract: Fast ignition with narrow-band coherent x-ray pulses has been revisited for cryogenic deuterium-tritium (DT) plasma conditions achieved on the OMEGA Laser System. In contrast to using hard-x-rays (hv = 3–6 keV) proposed in the original x-ray fast-ignition proposal, we find that soft-x-ray sources with hv ≈ 500 eV photons can be suitable for igniting the dense DT-plasmas achieved on OMEGA. Two-dimensional radiation–hydrodynamics simulations have identified the break-even conditions for realizing such a “hybrid”… Show more

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Cited by 6 publications
(2 citation statements)
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“…The formula is subsequently modified to the widely used form of E ig = 140 ( ρ 100 g cm −3 ) − 1.85 kJ by 2D simulations and the ignition window in the energy, power and intensity space is discussed [19]. Recent studies claim the ignition energy can be as low as 1 kJ when ρr h ≈ 0.36 g cm −2 , T ≈ 20 keV, ρ ⩾ 700 g cm −2 with non-thermal soft x-rays as the heating source [20,21]. Most previous studies on the isochoric fast ignition model assumed hot spots in the spherical center of the fuel.…”
Section: Introductionmentioning
confidence: 99%
“…The formula is subsequently modified to the widely used form of E ig = 140 ( ρ 100 g cm −3 ) − 1.85 kJ by 2D simulations and the ignition window in the energy, power and intensity space is discussed [19]. Recent studies claim the ignition energy can be as low as 1 kJ when ρr h ≈ 0.36 g cm −2 , T ≈ 20 keV, ρ ⩾ 700 g cm −2 with non-thermal soft x-rays as the heating source [20,21]. Most previous studies on the isochoric fast ignition model assumed hot spots in the spherical center of the fuel.…”
Section: Introductionmentioning
confidence: 99%
“…A properly assembled core with an extremely high pressure (>100-300 Gbar) makes it possible to produce not only sufficient a particles from DT fusions but also to "bootstrap" the heat (a-particle stopping) in the hot spot. 7 If this occurs, a fusion burn wave could quickly propagate through the dense shell 8 and net energy gain is expected.…”
Section: Introductionmentioning
confidence: 99%