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

Josiah B. Lewis; Dieter Isheim; Christine Floss; David N. Seidman

doi:10.1016/j.ultramic.2015.05.021

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

Josiah B. Lewis^*, Dieter Isheim, Christine Floss, David N. Seidman

^*Corresponding author for this work

Materials Science and Engineering

Research output: Contribution to journal › Article › peer-review

23 Scopus citations

Abstract

The astrophysical origins of ~3nm-diameter meteoritic nanodiamonds can be inferred from the ratio of ¹²C/¹³C. 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.

Original language	English (US)
Pages (from-to)	248-254
Number of pages	7
Journal	Ultramicroscopy
Volume	159
DOIs	https://doi.org/10.1016/j.ultramic.2015.05.021
State	Published - Dec 1 2015

Keywords

Atom-probe tomography
FIB liftout
Meteoritic nanodiamond
Nucleosynthesis
Presolar grains

ASJC Scopus subject areas

Electronic, Optical and Magnetic Materials
Atomic and Molecular Physics, and Optics
Instrumentation

Access to Document

10.1016/j.ultramic.2015.05.021

Cite this

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title = "12C/13C-ratio determination in nanodiamonds by atom-probe tomography",

abstract = "The astrophysical origins of ~3nm-diameter meteoritic nanodiamonds can be inferred from the ratio of 12C/13C. 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.",

keywords = "Atom-probe tomography, FIB liftout, Meteoritic nanodiamond, Nucleosynthesis, Presolar grains",

author = "Lewis, {Josiah B.} and Dieter Isheim and Christine Floss and Seidman, {David N.}",

note = "Funding Information: The LEAP tomograph at NUCAPT was acquired and upgraded with equipment grants from the NSF-MRI program (DMR-0420532) and NRL-DURIP (N00014-0400798, N00014-0610539, N00014-0910781). Funding Information: This work made use of the EPIC facility (NUANCE Center-Northwestern University), which has received support from the MRSEC program (NSF DMR-1121262) at the Materials Research Center; the Nanoscale Science and Engineering Center (NSF EEC–0647560) at the International Institute for Nanotechnology; and the State of Illinois, through the International Institute for Nanotechnology. Funding Information: This work is supported by NASA Grant NNX13AF53G (C.F.) . Publisher Copyright: {\textcopyright} 2015 Elsevier B.V.",

year = "2015",

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doi = "10.1016/j.ultramic.2015.05.021",

language = "English (US)",

volume = "159",

pages = "248--254",

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AU - Lewis, Josiah B.

AU - Isheim, Dieter

AU - Floss, Christine

AU - Seidman, David N.

N1 - Funding Information: The LEAP tomograph at NUCAPT was acquired and upgraded with equipment grants from the NSF-MRI program (DMR-0420532) and NRL-DURIP (N00014-0400798, N00014-0610539, N00014-0910781). Funding Information: This work made use of the EPIC facility (NUANCE Center-Northwestern University), which has received support from the MRSEC program (NSF DMR-1121262) at the Materials Research Center; the Nanoscale Science and Engineering Center (NSF EEC–0647560) at the International Institute for Nanotechnology; and the State of Illinois, through the International Institute for Nanotechnology. Funding Information: This work is supported by NASA Grant NNX13AF53G (C.F.) . Publisher Copyright: © 2015 Elsevier B.V.

PY - 2015/12/1

Y1 - 2015/12/1

N2 - The astrophysical origins of ~3nm-diameter meteoritic nanodiamonds can be inferred from the ratio of 12C/13C. 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.

AB - The astrophysical origins of ~3nm-diameter meteoritic nanodiamonds can be inferred from the ratio of 12C/13C. 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.

KW - Atom-probe tomography

KW - FIB liftout

KW - Meteoritic nanodiamond

KW - Nucleosynthesis

KW - Presolar grains

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