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Search indexed NASA NTRS and DOE OSTI research on propulsion, heat transfer, battery materials and energy systems. Follow report and document links to the original sources.

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131 records · Page 8
All sourcesNASA NTRSDOE OSTI
NASA NTRS2017

Single-Step, Solvent-Free, Catalyst-Free Preparation of Holey Carbon Allotropes

Methods for forming holey carbon allotropes and graphene nanomeshes are provided by the various embodiments. The various embodiments may be applicable to a variety of carbon allotropes, such as graphene, graphene oxide, reduced graphene oxide, thermal exfoliated graphene, graphene nanoribbons, graphite, exfoliated graphite, expanded graphite, carbon nanotubes (e.g., single-walled carbon nanotubes, double-walled carbon nanotubes, few-walled carbon nanotubes, multi-walled carbon nanotubes, etc.), carbon nanofibers, carbon fibers, carbon black, amorphous carbon, fullerenes, etc. The methods may produce holey carbon allotropes without the use of solvents, catalysts, flammable gas, additional chemical agents, or electrolysis to produce the pores (e.g., holes, etc.) in the carbon allotropes. In an embodiment, a carbon allotrope may be heated at a working window temperature for a working period of time to create holes in the carbon allotrope.

Lin, Yi↗
NASA NTRS2018

Interstellar PAHs: From Ground to Space, Expanding Spectroscopic Frontiers

Recent progress in astrochemistry and in our understanding of the Molecular Universe has been driven by new detector technologies and advances in ground-, airborne- and space astronomy coupled to new, innovative approaches in molecular spectroscopy. The search for the complex carbon-based molecules (PAHs, Fullerenes, nanoparticles) thought to be responsible for the ubiquitous infrared emission bands (UIBs) and optical absorption bands (DIBs) that are observed in various regions of the interstellar medium of local- and extragalactic environments illustrates the progress in spectroscopy techniques that has been driven by astronomy. Recent progresses reached in this domain will be discussed together with the laboratory techniques that have been developed to measure the spectra of laboratory analogs of cosmic molecules in the UV Visible-NIR range under experimental conditions that attempt to reproduce the interstellar conditions.

Laboratory astrophysics and astrochemistry↗
NASA NTRSDate not supplied

Polycyclic aromatic hydrocarbons (PAHs)

Polycyclic aromatic hydrocarbons (PAHs) are the most abundant, large, carbon-based, molecular species in the interstellar medium (ISM). They are responsible for a series of prominent infrared (IR) emission features that dominate the IR spectra of many astronomical sources. The recent detection of cyano-naphthalene in TMC-1 (molecular cloud) and fullerenes in Tc 1 (planetary nebula) bracket the presumed evolutionary pathway of astronomical PAHs; from their formation to ending up in their most-stable forms. Furthermore, their discovery indicates a rich, complex ongoing PAH chemistry. Significant progress has been made in connecting the (photo)chemical evolution of the astronomical PAH population to variations observed in the interstellar PAH IR bands. Subsequently, these variations have been tied to distinct stages of the stellar life-cycle. However, questions remain regarding some components of the astronomical PAH IR emission spectrum. One concerns the origin and evolution of the weaker plateaus that sit beneath the main features and extend from roughly 3.2-3.6, 6-9, 11-15, and 15-20 µm. Observations from JWST will provide the opportunity to investigate subtle changes in the PAH IR bands with unprecedented sensitivity. This presents an exciting opportunity for the field of astrochemistry.

Polycyclic aromatic hydrocarbons;↗
NASA NTRS1993

Synthesis of C60H2 by rhodium-catalyzed hydrogenation of C60

Reduction of C60 with rhodium(0) on alumina and hydrogen in deuterated benzene (C6D6) at ambient temperature and pressure yields a mixture of hydrogenated compounds; C60H2 has been characterized as the major product in 14% yield based on 1H NMR.

Non-NASA Center↗