NASA Logo

NTRS

NTRS - NASA Technical Reports Server

Press Enter or click the Search button to begin your search.

Back to Results
Electronic and molecular structure of carbon grainsClusters of carbon atoms have been studied with large-scale ab initio calculations. Planar, single-sheet graphite fragments with 6 to 54 atoms were investigated, as well as the spherical C(sub 60) Buckminsterfullerene molecule. Polycyclic aromatic hydrocarbons (PAHs) have also been considered. Thermodynamic differences between diamond- and graphite-like grains have been studied in particular. Saturation of the peripheral bonds with hydrogen is found to provide a smooth and uniform convergence of the properties with increasing cluster size. For the graphite-like clusters the convergence to bulk values is much slower than for the three-dimensional complexes.
Document ID
19900018258
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Almloef, Jan
(Minnesota Univ. Minneapolis, MN, United States)
Luethi, Hans-Peter
(Minnesota Univ. Minneapolis, MN, United States)
Date Acquired
September 6, 2013
Publication Date
April 1, 1990
Publication Information
Publication: NASA, Ames Research Center, Carbon in the Galaxy: Studies from Earth and Space
Subject Category
Astrophysics
Accession Number
90N27574
Funding Number(s)
CONTRACT_GRANT: NSF CHE-86-10809
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
No Preview Available