4.4 Article Proceedings Paper

12C/13C ratio determination in nanodiamonds by atom-probe tomography

期刊

ULTRAMICROSCOPY
卷 159, 期 -, 页码 248-254

出版社

ELSEVIER
DOI: 10.1016/j.ultramic.2015.05.021

关键词

Atom-probe tomography; Meteoritic nanodiamond; Presolar grains; Nucleosynthesis; FIB liftout

资金

  1. NASA [NNX13AF53G]
  2. NSF-MRI program [DMR0420532]
  3. NRL-DURIP [N00014-0400798, N00014-0610539, N00014-0910781]
  4. MRSEC program at the Materials Research Center [NSF DMR-1121262]
  5. Nanoscale Science and Engineering Center at the International Institute for Nanotechnology [NSF EEC0647560]
  6. State of Illinois, through the International Institute for Nanotechnology
  7. Initiative for Sustainability and Energy at Northwestern
  8. NASA [NNX13AF53G, 474493] Funding Source: Federal RePORTER

向作者/读者索取更多资源

The astrophysical origins of similar to 3 nm-diameter meteoritic nanodiamonds can be inferred from the ratio of C-12/C-13. It is essential to achieve high spatial and mass resolving power and minimize all sources of signal loss in order to obtain statistically significant measurements. We conducted atom-probe tomography on meteoritic nanodiamonds embedded between layers of Pt. We describe sample preparation, atom-probe tomography analysis, 3D reconstruction, and bias correction. We present new data from meteoritic nanodiamonds and terrestrial standards and discuss methods to correct isotopic measurements made with the atom-probe tomograph. (C) 2015 Elsevier B.V. All rights reserved.

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