1992
DOI: 10.1016/0022-4073(92)90085-i
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Free-free emission continuum of weakly non-ideal argon plasmas

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Cited by 6 publications
(11 citation statements)
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“…We are led to a difference equal to ∆ 1 + ∆ 2 = δz between reaching the "entrance" point x e,− (for F ) relative to the "entrance-exit" point xa (for Fa), leading to an energy uncertainty ∆E = abs(−Ip − δz) = (I b + δ), for F ≤ Fa, and with a time τ T,i (F ) = for arbitrary subatomic field strength F , hence one obtains eq (20) instead of eq. (19). We have explained so far eq (17) and eq (20), in doing so we explained the physical meaning of the symmetry consideration done above (see eq (15) and the discussion before) and we obtain from eqs (17), (20) the result obtained in eq (15):…”
Section: Total Time For Subatomic Field F < F Amentioning
confidence: 99%
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“…We are led to a difference equal to ∆ 1 + ∆ 2 = δz between reaching the "entrance" point x e,− (for F ) relative to the "entrance-exit" point xa (for Fa), leading to an energy uncertainty ∆E = abs(−Ip − δz) = (I b + δ), for F ≤ Fa, and with a time τ T,i (F ) = for arbitrary subatomic field strength F , hence one obtains eq (20) instead of eq. (19). We have explained so far eq (17) and eq (20), in doing so we explained the physical meaning of the symmetry consideration done above (see eq (15) and the discussion before) and we obtain from eqs (17), (20) the result obtained in eq (15):…”
Section: Total Time For Subatomic Field F < F Amentioning
confidence: 99%
“…The time reduction in τ (x i , x e,− ) for F comparing to τ (x i , xa) = 1/(2Ip) for Fa, eq (19), is a factor depending on δz (see discussion after eq (16)), because the kinetic energy experiences a change proportional to (x e,− − x i ) F < (xa − x i ) Fa. A (weaker) field F < Fa is not sufficient to compensate for the kinetic energy at the (shake-up) step, instead the electron is at the "entrance"…”
Section: Total Time For Subatomic Field F < F Amentioning
confidence: 99%
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“…Since much of this type of radiation in the visible and ultraviolet is generated near the nucleus, expression (16) is believed to underestimate the radiation intensities when Z > Z eff , especially if Z ¾ 1. In studies that are not related to sonoluminescence, eVorts are known to better describe the radiation intensity if Z > 1, see for example [105,195,196]. (3) Recombination radiation.…”
Section: Extensions and Outlookmentioning
confidence: 99%