By B. L. van der Waerden
Most vital early papers through Einstein, Bohr, Born, Heisenberg, Dirac and Pauli-covering interval from 1917-26.
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Under these conditions, the beginning of the plateau region is at the same velocity: γ ∗ ≈ γ 0 . But if ε1 is smaller than 1, as happens for energies E above the highest resonances of the atoms of the medium, then there is no Cerenkov light to correspond to the onset of the plateau. g. [JAC 75]): ωp2 = 4π Ne2 /m. 62) 1 − ε1 (ω ). 59), the beginning of the plateau is given by the plasma frequency for every value E of the energy loss: γ ∗ ≈ ω /ωp = m 4π Nc2 1/2 E . 63) It turns out that this relation (which was derived for a free-electron gas) already holds very well for all E above the M-shell resonances in argon.
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P. Young, Resonance ionization spectro– scopy and one-atom detection, Rev. Mod. Phys. 51, 767 (1979) M. Inokuti, Ionization yields in gases under electron irradiation, Radiat. Res. D. Jackson, Classical electrodynamics, 2nd edn (Wiley, New York 1975) E. J. Kobetich and R. Katz, Energy deposition by electron beams and delta rays, Phys. Rev. S. K¨olbig and B. Schorr, A program package for the Landau distribution, Comput. Phys. Commun. 31, 97 (1984) P. Lambropoulos, Topics in multiphoton processes in atoms, Adv.
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