Photoionization and Other Probes of Many - Electron Interactions 1976
DOI: 10.1007/978-1-4684-2799-8_13
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Ionization by Nuclear Transitions

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Cited by 4 publications
(5 citation statements)
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“…When an α-particle passes the fast inner atomic electrons, the direct collision process can lead to the emission of a shake-off electron [26][27][28]. The resulting electron energy spectrum shows a higher-order potential dependence [29] because the decay energy is shared between the α-particle and the emitted electron, which carries only a small fraction, usually of the same order of magnitude as the shell binding energy E b .…”
Section: Particle Generationmentioning
confidence: 99%
“…When an α-particle passes the fast inner atomic electrons, the direct collision process can lead to the emission of a shake-off electron [26][27][28]. The resulting electron energy spectrum shows a higher-order potential dependence [29] because the decay energy is shared between the α-particle and the emitted electron, which carries only a small fraction, usually of the same order of magnitude as the shell binding energy E b .…”
Section: Particle Generationmentioning
confidence: 99%
“…A nuclear α-decay leads to a perturbation of the atomic shells, as the electrons experience the passage of the outgoing α-particle through the atomic orbitals, as well as the sudden change ∆Z = Z − Z of the Coulomb potential of the nucleus (initial state: Z = 86 for radon, final state: Z = 84 for polonium) [20]. The impact of both processes on innershell (K, L, M) electrons is different than on outer-shell (N or higher) electrons due to the largely different orbital velocities.…”
Section: Inner Shell Shake-off Processesmentioning
confidence: 99%
“…For inner shells, electron shake-off (SO) is caused by the direct collision process [20,21,22]. In this case, the α-particle, which has already gained 99% of its final kinetic Table 1: The table gives an overview of the relative probabilities P i (per α-decay) of the dominant IC lines and of the corresponding electron energies E kin for 219 Rn, as measured by [18].…”
Section: Inner Shell Shake-off Processesmentioning
confidence: 99%
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“…Sources of primary stored electrons include β-decays of tritium molecules (HT, T 2 ) and processes occurring during α-decays of the radon isotopes 219,220 Rn. The energy distribution of these primary electrons varies by more than five orders of magnitude from the eV level up to about one hundred keV [22][23][24][25][26][27][28]. However, in terms of cyclotron frequency f c (B, γ) this implies a variation of about 20% (1 ≤ γ ≤ 1.2) only.…”
Section: The Working Principle Of Ecr At a Katrin Spectrometermentioning
confidence: 99%