| Literature DB >> 26095824 |
Josiah B Lewis1, Dieter Isheim2, Christine Floss3, David N Seidman2.
Abstract
The astrophysical origins of ∼ 3 nm-diameter meteoritic nanodiamonds can be inferred from the ratio of C12/C13. 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.Entities:
Keywords: Atom-probe tomography; FIB liftout; Meteoritic nanodiamond; Nucleosynthesis; Presolar grains
Year: 2015 PMID: 26095824 DOI: 10.1016/j.ultramic.2015.05.021
Source DB: PubMed Journal: Ultramicroscopy ISSN: 0304-3991 Impact factor: 2.689