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84894012668
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note
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0 functions oscillate in phase in the real part when β ≈ α/q. 26. This result is, of course, well known for rectangular density profiles. (See Ref. 24.) 27. Another system fulfilling these conditions is krypton at λ ≈ 348 nm and λ ≈ 369 nm. Interesting differences between Gaussian and noncollinear beams have been described for resonant harmonic generation and multiphoton ionization in xenon at λ ≈ 440 nm. (See Ref. 7.)
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30
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We verified this by evaluating the contribution of pressure broadening to the absorption coefficient, for hydrogen and xenon at 355 nm, in the simple approaches of W. R. Ferrell, M. G. Payne, and W. R. Garrett, "Resonance broadening and shifting of spectral lines in xenon and krypton," Phys. Rev. A 36, 81-89 (1987); and of G. Peach, "Collisional broadening of spectral lines," in Atomic, Molecular, and Optical Physics Handbook, G. W. F. Drake, ed. (American Institute of Physics, Melville, New York, 1996), p. 669, Eq. (57.27).
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