A procedure for measuring the helium density and pressure in nanometre-sized bubbles in irradiated materials using electron-energy-loss spectroscopy

Citation
Ca. Walsh et al., A procedure for measuring the helium density and pressure in nanometre-sized bubbles in irradiated materials using electron-energy-loss spectroscopy, PHIL MAG A, 80(7), 2000, pp. 1507-1543
Citations number
67
Categorie Soggetti
Apllied Physucs/Condensed Matter/Materiales Science
Journal title
PHILOSOPHICAL MAGAZINE A-PHYSICS OF CONDENSED MATTER STRUCTURE DEFECTS ANDMECHANICAL PROPERTIES
ISSN journal
13642804 → ACNP
Volume
80
Issue
7
Year of publication
2000
Pages
1507 - 1543
Database
ISI
SICI code
1364-2804(200007)80:7<1507:APFMTH>2.0.ZU;2-F
Abstract
A procedure for measuring the density of He in nanometre-sized bubbles in m aterials using electron-energy-loss spectroscopy is given. Tt involves meas uring the scattering probability of an electron as a result of exciting a I s electron in He to the 2p state. An expression for the cross-section of th is interaction is obtained, taking into account some relativistic effects, the q dependence of the matrix element and the effect of a non-zero converg ence angle of the incident electron beam. An accuracy of about 10% in the c alculation of the He density can be achieved using this technique. The proc edure is demonstrated using spectra obtained from He bubbles in irradiated PE16 alloy specimens and used to make preliminary investigations into the r elationship between the blue shift of the 1s --> 2p transition in lie with atomic density and the relationship between the pressure in the bubbles and the bubble radius. The best estimate of the pressure in the We bubbles sho ws it to be less than half that required to achieve equilibrium with the su rface tension of the metal, if the usually accepted value of the surface te nsion is used. The blue shifts observed for bubbles of diameter 50 and 250 Angstrom can be extrapolated, within experimental error, to those obtained by Jager et al. for much higher helium densities.