Magnetic field and electromagnetic wave properties of carbon monoxide with high-pressure disproportionation single-walled carbon nanotubes
Creators
- 1. Department of Physics, Laboratory of Materials and Nanotechnology and Laboratory of Applied Physics, Amirkabir University of Technology (Tehran Polytechnic), Tehran P.O. Box 15875-4413 (Iran, Islamic Republic of)
Description
A double-fluid theory is used to find the electromagnetic wave absorption of carbon monoxide with iron-catalyzed high-pressure disproportionation (HiPco)-grown single-walled carbon nanotubes (SWNTs). The electromagnetic wave absorption of carbon monoxide with HiPco SWNTs is obtained and is studied numerically. The absorption is then deduced and their functional dependence on the number density, collision frequency, cyclotron frequency, and angle of propagation is studied. The double-fluid theory predicts that there is an electromagnetic frequency dependency on the energy absorption properties of the system under investigation. The calculation results show that effects of magnetic field strength and the angle of microwave propagation on the absorption coefficient as well as the frequency band of resonant absorption are very significant.
Additional details
Identifiers
- DOI
- 10.1063/1.3247075;
Publishing Information
- Journal Title
- Physics of Plasmas
- Journal Volume
- 16
- Journal Issue
- 10
- Journal Page Range
- p. 103302-103302.7
- ISSN
- 1070-664X
- CODEN
- PHPAEN
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 41021658
- Subject category
- S70: PLASMA PHYSICS AND FUSION TECHNOLOGY; S36: MATERIALS SCIENCE;
- Descriptors DEI
- CARBON; CARBON MONOXIDE; ENERGY ABSORPTION; MAGNETIC FIELDS; MICROWAVE RADIATION; NANOTUBES; OXIDATION; PLASMA WAVES
- Descriptors DEC
- ABSORPTION; CARBON COMPOUNDS; CARBON OXIDES; CHALCOGENIDES; CHEMICAL REACTIONS; ELECTROMAGNETIC RADIATION; ELEMENTS; NANOSTRUCTURES; NONMETALS; OXIDES; OXYGEN COMPOUNDS; RADIATIONS; SORPTION
Optional Information
- Notes
- (c) 2009 American Institute of Physics