
Proceedings Paper
Achieving zero stress in iridium, chromium, and nickel thin filmsFormat | Member Price | Non-Member Price |
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Paper Abstract
We examine a method for achieving zero intrinsic stress in thin films of iridium, chromium, and nickel deposited by magnetron sputter deposition. The examination of the stress in these materials is motivated by efforts to advance the optical performance of light-weight x-ray space telescopes into the regime of sub-arc second resolution. A characteristic feature of the intrinsic stress behavior in chromium and nickel is their sensitivity to the magnitude and sign of the intrinsic stress with argon gas pressure, including the existence of a critical pressure that results in zero film stress. This critical pressure scales linearly with the film’s density. While the effect of stress reversal with argon pressure has been previously reported by Hoffman and others for nickel and chromium, we have discovered a similar behavior for the intrinsic stress in iridium films. Additionally, we have identified zero stress in iridium shortly after island coalescence in the high adatom mobility growth regime. This feature of film growth is used for achieving a total internal stress of -2.89 MPa for a 15.8 nm thick iridium film with a surface roughness of 5.0 ± 0.5Å based on x-ray reflectivity (XRR) measurement at CuKα. The surface topography was also examined using atomic force microscopy (AFM). The examination of the stress in these films has been performed with a novel in-situ measurement device. The methodology and sensitivity of the in-situ instrument is also described herein.
Paper Details
Date Published: 12 May 2015
PDF: 15 pages
Proc. SPIE 9510, EUV and X-ray Optics: Synergy between Laboratory and Space IV, 95100E (12 May 2015); doi: 10.1117/12.2180641
Published in SPIE Proceedings Vol. 9510:
EUV and X-ray Optics: Synergy between Laboratory and Space IV
René Hudec; Ladislav Pina, Editor(s)
PDF: 15 pages
Proc. SPIE 9510, EUV and X-ray Optics: Synergy between Laboratory and Space IV, 95100E (12 May 2015); doi: 10.1117/12.2180641
Show Author Affiliations
David M. Broadway, NASA Marshall Space Flight Ctr. (United States)
Jeffrey Weimer, The Univ. of Alabama in Huntsville (United States)
Danielle Gurgew, The Univ. of Alabama in Huntsville (United States)
Tomasz Lis, The Univ. of Alabama in Huntsville (United States)
Brian D. Ramsey, NASA Marshall Space Flight Ctr. (United States)
Jeffrey Weimer, The Univ. of Alabama in Huntsville (United States)
Danielle Gurgew, The Univ. of Alabama in Huntsville (United States)
Tomasz Lis, The Univ. of Alabama in Huntsville (United States)
Brian D. Ramsey, NASA Marshall Space Flight Ctr. (United States)
Stephen L. O'Dell, NASA Marshall Space Flight Ctr. (United States)
Mikhail Gubarev, NASA Marshall Space Flight Ctr. (United States)
A. Ames, Smithsonian Astrophysics Observatory (United States)
R. Bruni, Smithsonian Astrophysics Observatory (United States)
Mikhail Gubarev, NASA Marshall Space Flight Ctr. (United States)
A. Ames, Smithsonian Astrophysics Observatory (United States)
R. Bruni, Smithsonian Astrophysics Observatory (United States)
Published in SPIE Proceedings Vol. 9510:
EUV and X-ray Optics: Synergy between Laboratory and Space IV
René Hudec; Ladislav Pina, Editor(s)
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