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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