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image/svg+xml Jakob Voss, based on art designer at PLoS, modified by Wikipedia users Nina and Beao Closed Access logo, derived from PLoS Open Access logo. This version with transparent background. http://commons.wikimedia.org/wiki/File:Closed_Access_logo_transparent.svg Jakob Voss, based on art designer at PLoS, modified by Wikipedia users Nina and Beao Physical Review Aarrow_drop_down
image/svg+xml Jakob Voss, based on art designer at PLoS, modified by Wikipedia users Nina and Beao Closed Access logo, derived from PLoS Open Access logo. This version with transparent background. http://commons.wikimedia.org/wiki/File:Closed_Access_logo_transparent.svg Jakob Voss, based on art designer at PLoS, modified by Wikipedia users Nina and Beao
Physical Review A
Article . 1993 . Peer-reviewed
License: APS Licenses for Journal Article Re-use
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Fast inelastic ion-ion, ion-electron, and ion-positron collisions

Authors: , Chidichimo; , Schranz; , Zygelman;

Fast inelastic ion-ion, ion-electron, and ion-positron collisions

Abstract

We present scaling relations for the total cross sections and collision strengths of bound-state excitation in positive ions. The colliding particle can be positively or negatively charged and can be a fully ionized atom, an electron, or a positron. We consider collisions in which the kinetic energy of relative motion is large and consequently the adiabaticity parameter \ensuremath{\xi}\ensuremath{\ll}1. We illustrate our general method by calculating collision strengths for proton-impact excitation of fine-structure transitions in hydrogenlike ions. The limiting case of infinite nuclear charge is also included in our calculations. Using a unitarized Coulomb-Born approximation, we show that, for dipole transitions, colliding particles with large orbital angular momenta (l\ensuremath{\gtrsim}2000) make an important contribution (\ensuremath{\sim}70%) to the collision strength of proton-impact excitation. For a nonrelativistic projectile energy ${\mathit{E}}_{\mathit{i}}$\ensuremath{\rightarrow}\ensuremath{\infty}, we use the Born approximation to obtain the scaled collision strengths. These limiting values, dependent only on the particular transition, confirm the correct high-energy behavior of our data. We also use the interactive graphics computer program omeups [Burgess and Tully, Astron. Astrophys. 254, 436 (1992)] to extrapolate our data to higher energies.

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selected citations
These citations are derived from selected sources.
This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Citations provided by BIP!
popularity
This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
BIP!Popularity provided by BIP!
influence
This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Influence provided by BIP!
impulse
This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
BIP!Impulse provided by BIP!
4
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