Absolute doubly differential angular sputtering yields for 20 keV Kr+ on polycrystalline Cu

Author:

Bu Caixia1ORCID,Morrissey Liam S.23ORCID,Bostick Benjamin C.4ORCID,Burger Matthew H.5ORCID,Bowen Kyle P.1ORCID,Chillrud Steven N.4ORCID,Domingue Deborah L.6ORCID,Dukes Catherine A.7ORCID,Ebel Denton S.8ORCID,Harlow George E.8ORCID,Hillenbrand Pierre-Michel1ORCID,Ivanov Dmitry A.1ORCID,Killen Rosemary M.2ORCID,Ross James M.4,Schury Daniel1ORCID,Tucker Orenthal J.2ORCID,Urbain Xavier9ORCID,Zhang Ruitian1ORCID,Savin Daniel W.1ORCID

Affiliation:

1. Columbia Astrophysics Laboratory, Columbia University 1 , New York, New York 10027, USA

2. NASA Goddard Space Flight Center 2 , Greenbelt, Maryland 20771, USA

3. Faculty of Engineering and Applied Science, Memorial University 3 , Newfoundland and Labrador A1B 3X7, Canada

4. Lamont-Doherty Earth Observatory, Columbia University 4 , Palisades, New York 10964, USA

5. Space Telescope Science Institute 5 , 3700 San Martin Dr., Baltimore, Maryland 21218, USA

6. Planetary Science Institute 6 , Tucson, Arizona 85719, USA

7. Laboratory for Astrophysics and Surface Physics, University of Virginia 7 , Charlottesville, Virginia 22904, USA

8. American Museum of Natural History 8 , New York, New York 10024, USA

9. Université Catholique de Louvain 9 B-1348 Louvain-la-Neuve, Belgium

Abstract

We have measured the absolute doubly differential angular sputtering yield for 20 keV Kr+ impacting a polycrystalline Cu slab at an incidence angle of θi = 45° relative to the surface normal. Sputtered Cu atoms were captured using collectors mounted on a half dome above the sample, and the sputtering distribution was measured as a function of the sputtering polar, θs, and azimuthal, ϕs, angles. Absolute results of the sputtering yield were determined from the mass gain of each collector, the ion dose, and the solid angle subtended, after irradiation to a total fluence of ∼1 × 1018 ions/cm2. Our approach overcomes shortcomings of commonly used methods that only provide relative yields as a function of θs in the incidence plane (defined by the ion velocity and the surface normal). Our experimental results display an azimuthal variation that increases with increasing θs and is clearly discrepant with simulations using binary collision theory. We attribute the observed azimuthal anisotropy to ion-induced formation of micro- and nano-scale surface features that suppress the sputtering yield through shadowing and redeposition effects, neither of which are accounted for in the simulations. Our experimental results demonstrate the importance of doubly differential angular sputtering studies to probe ion sputtering processes at a fundamental level and to explore the effect of ion-beam-generated surface roughness.

Funder

NASA SSW

NIH

NSF

Publisher

AIP Publishing

Subject

General Physics and Astronomy

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