Unreliability of the autocorrelation function as evidence for Ericson fluctuations
- 1. Institut fuer Experimentalphysik, Freie Universitaet Berlin, Arnimallee 14, D-14195 Berlin-Dahlem (Germany)
- 2. Laboratoire Kastler-Brossel, Universite Pierre et Marie Curie-Paris 6, ENS, CNRS, 4 Place Jussieu, F-75005 Paris (France)
Description
In a recent combined experimental and theoretical paper for the total photoionization cross section of helium up to the single-ionization threshold I13, we had shown that Ericson fluctuations were absent, although the Ericson regime had already been reached. In the present paper, we study the autocorrelation functions of the total photoionization cross section below I9--I13 and find that these are essentially identical to that of an artificial spectrum with Ericson fluctuations. Consequently, we have to conclude that the autocorrelation function alone--although its Lorentzian-like shape for small displacements ε has been used by some authors--is a necessary but is not a sufficient proof for the existence of Ericson fluctuations. In the present case of He, the absence of Ericson fluctuations is a consequence of a strong hierarchy between the transitions belonging to different series with approximate quantum numbers that still exist in this region; this causes the spectra to be dominated by the principal series.
Additional details
Identifiers
Publishing Information
- Journal Title
- Physical Review. A
- Journal Volume
- 84
- Journal Issue
- 2
- Journal Page Range
- p. 023402-023402.6
- ISSN
- 1050-2947
- CODEN
- PLRAAN
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 44034568
- Subject category
- S74: ATOMIC AND MOLECULAR PHYSICS; S71: CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS;
- Descriptors DEI
- CORRELATIONS; CROSS SECTIONS; ERICSON THEORY; FUNCTIONS; HELIUM; PHOTOIONIZATION; QUANTUM NUMBERS; SPECTRA
- Descriptors DEC
- ELEMENTS; FLUIDS; GASES; IONIZATION; NONMETALS; RARE GASES
Optional Information
- Notes
- (c) 2011 American Institute of Physics