2007
DOI: 10.1088/0953-4075/40/22/f01
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Temperature enhancement of Xe(L) x-ray amplifier (λ ∼ 2.9 Å) emission

Abstract: Cooling of the xenon nozzle flow to T = 230 K produces three leading effects. They are (1) a ∼2.5-fold enhancement of the Xe(L) hollow atom emission on the single-vacancy 3d → 2p charge state arrays, (2) the production of amplifying self-trapped plasma channels with significantly enhanced lengths and (3) very sharply augmented emission on (2s2p) Xe(L) double-vacancy transitions in the λ ∼ = 2.80 Å region.

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Cited by 13 publications
(18 citation statements)
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“…A non-equilibrium dynamics model of xenon was constructed to determine conditions under which population inversions would be generated within several inner-shell pathways that would produce comparable amounts of X-ray amplification as had been observed experimentally at w2.8 Å [24,28] (and the references therein). In the modeling of these experiments, clusters of xenon atoms were found to be rapidly stripped of all N-shell electrons on a femtosecond time scale by a light pulse of 5 eV photons focused to peak intensities slightly greater than 10 19 W/cm 2 .…”
Section: Discussionmentioning
confidence: 99%
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“…A non-equilibrium dynamics model of xenon was constructed to determine conditions under which population inversions would be generated within several inner-shell pathways that would produce comparable amounts of X-ray amplification as had been observed experimentally at w2.8 Å [24,28] (and the references therein). In the modeling of these experiments, clusters of xenon atoms were found to be rapidly stripped of all N-shell electrons on a femtosecond time scale by a light pulse of 5 eV photons focused to peak intensities slightly greater than 10 19 W/cm 2 .…”
Section: Discussionmentioning
confidence: 99%
“…[24,28] experiments, the expansion and heating dynamics were coupled to the ionization dynamics as depicted schematically in Fig. 5.…”
Section: The Coupling Cluster and Ionization Dynamics Laserecluster mentioning
confidence: 99%
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“…that defines the peak electric field E for the onset of relativistic motions for elections with mass m and charge e driven at angular frequency ω, (b) the vacuum pair creation limit, the upper value bounding the achievable intensity that is associated with ultrarelativistic electron/positron cascades [97], (c) the intensity I  4.6 × 10 29 W/cm 2 corresponding to the Schwinger/Heisenberg limit [98,99], and (d) the point characterizing the intensity of saturated amplification with the Xe(L) hollow atom system [38,39,[61][62][63][64][65][66].…”
mentioning
confidence: 99%