Light emission from an oxygen covered copper surface by ion bombardment

Citation
Cs. Lee et al., Light emission from an oxygen covered copper surface by ion bombardment, SURF SCI, 488(3), 2001, pp. 379-386
Citations number
38
Categorie Soggetti
Physical Chemistry/Chemical Physics
Journal title
SURFACE SCIENCE
ISSN journal
00396028 → ACNP
Volume
488
Issue
3
Year of publication
2001
Pages
379 - 386
Database
ISI
SICI code
0039-6028(20010810)488:3<379:LEFAOC>2.0.ZU;2-I
Abstract
Light emission from oxygen covered metal surface is used to investigate the sputtering yield, So, and the sticking coefficient, cs, of oxygen atoms on the surface of a polycrystalline copper target. The spectral lines of Cu I emitted from sputtered excited atoms under Ar+ and Ne+ ion bombardment of a polycrystalline copper target are measured as a function of the oxygen pa rtial pressure, wavelength and beam energy. The light emission for two Cu I lines (3247 and 3274 Angstrom) are proportional to the oxygen partial pres sure (similar to1 X 10(4) Torr). Above 2 x 10(-4) Torr, the light intensiti es start to decrease in accordance with observations in other metal measure ments. The intensities of Cu I spectral lines are measured as a function of time and oxygen partial pressures, and the sputtering yields and the stick ing coefficient are determined from the curves of spectral lines directly. For 10 and 20 keV AC ions bombarded the copper surface, the oxygen sputteri ng yields from the copper surface are 0.34 and 0.22 respectively. For Ne+ i ons with 5 and 10 keV, the oxygen sputtering yields are 0.87 and 0.59 respe ctively. The sticking coefficient of oxygen atoms on the copper surface is constant in all measurements and is estimated as around (2.34 +/- 0.49) x 1 0(-3). Combined results with this experiment and a previous measurement [Su rf. Sci. 471 (2000) 219-24], we believe that beam induced light emission is a useful technique to measure the oxygen-sticking coefficient on metal sur faces. (C) 2001 Elsevier Science B.V. All rights reserved.