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For neon, computations based on electron-impact ionization agree very well with the experiments. For other species, such as argon, excitation tunneling should also be considered [V. L. B. de Jesus et al. (unpublished)].
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47
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85032426961
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note
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1). This interaction is implicit in Eq. (7). For other types of interactions see, e.g., Ref. [14].
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48
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0142188735
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The start and return times coalesce at the maximal and minimal classically allowed momenta, denning a confined phase-space region. See, e.g., C. Figueira de Morisson Faria and W. Becker, Laser Phys. 13, 1196 (2003).
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85032429629
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Longer excursion times are not relevant due to wave-packet spreading, which makes the overlap between the wave packets of the first and of the second electrons negligible. In our classical model, this implies leaving the corresponding electrons out of the ensemble.
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50
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85032427631
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note
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Other sets of electrons practically do not contribute to the yield, since the corresponding tunneling rate is very small. Their influence is seen if this rate is artificially taken to be constant (cf. lower panels of Fig. 1).
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51
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85032430847
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note
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Other sets of electrons practically do not contribute to the yield, since the corresponding tunneling rate is very small. Their influence is seen if this rate is artificially taken to be constant (cf. lower panels of Fig. 1).
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85032426341
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C. Figueira de Morisson Faria et al. (to be published)
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C. Figueira de Morisson Faria et al. (to be published).
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