Five-Membered Loop-Initiated Nucleation of Unlayered Graphene Sheets in a Carbon Melt, with Diffusion Barrier Possibilities
A subset of isotopically “presolar” carbon particles extracted from the Murchison meteorite
contain signatures expected of particles formed in the atmosphere of red giant stars. Some …
contain signatures expected of particles formed in the atmosphere of red giant stars. Some …
A Semi-empirical Model for the Containerless Solidification of Liquid Carbon
P Chrostoski, C Silva, R Molitor… - The Journal of Physical …, 2023 - ACS Publications
Elemental carbon has important structural diversity, ranging from nanotubes through
graphite to diamond. Transmission electron microscope studies of micron-size core/rim …
graphite to diamond. Transmission electron microscope studies of micron-size core/rim …
DFT study of “unlayered graphene solid” formation, in liquid carbon droplets at low pressures
This atomistic modeling study is companion to new experimental work on carbon vapor slow-
cooled in (a) the laboratory and (b) the atmosphere of ancient carbon-synthesizing stars. It …
cooled in (a) the laboratory and (b) the atmosphere of ancient carbon-synthesizing stars. It …
The rates of unlayered graphene formation in a supercooled carbon melt at low pressure
Elemental carbon has important structural diversity, ranging from nanotubes to graphite and
diamond. Studies of primitive meteorite extracted micron-size core/rim carbon spheres …
diamond. Studies of primitive meteorite extracted micron-size core/rim carbon spheres …
Modeling graphene sheet growth and dynamical matrix calculations using molecular dynamics
VH Vattikuti, P Chrostoski - 2024 - osti.gov
Molecular dynamics (MD) has been an incredibly useful tool to model physical processes
that were synthesized experimentally but not fully understood. MD, through the use of semi …
that were synthesized experimentally but not fully understood. MD, through the use of semi …
[图书][B] Computational studies of carbon nanocluster solidification
CC Silva - 2021 - search.proquest.com
A subset of micron-size meteoritic carbon particles formed in red giant atmospheres show a
core-rim structure, likely condensed from a vapor phase into super-cooled carbon droplets …
core-rim structure, likely condensed from a vapor phase into super-cooled carbon droplets …