NASA Logo

NTRS

NTRS - NASA Technical Reports Server

Back to Results
Carbon Nanotubes for Space Photovoltaic ApplicationsCarbon nanotubes (CNTs) can be envisioned as an individual graphene sheet rolled into a seamless cylinder (single-walled, SWNT), or concentric sheets as in the case of a multi-walled carbon nanotube (MWNT) (1). The role-up vector will determine the hexagonal arrangement and "chirality" of the graphene sheet, which will establish the nanotube to be metallic or semiconducting. The optoelectronic properties will depend directly on this chiral angle and the diameter of the SWNT, with semiconductor types exhibiting a band gap energy (2). Characteristic of MWNTs are the concentric graphene layers spaced 0.34 nm apart, with diameters from 10-200 nm and lengths up to hundreds of microns (2). In the case of SWNTs, the diameters range from 0.4 - 2 nm and lengths have been reported up to 1.5 cm (3). SWNTs have the distinguishable property of "bundling" together due to van der Waal's attractions to form "ropes." A comparison of these different structural types is shown in Figure 1. The use of SWNTS in space photovoltaic (PV) applications is attractive for a variety of reasons. Carbon nanotubes as a class of materials exhibit unprecedented optical, electrical, mechanical properties, with the added benefit of being nanoscale in size which fosters ideal interaction in nanomaterial-based devices like polymeric solar cells. The optical bandgap of semiconducting SWNTs can be varied from approx. 0.4 - 1.5 eV, with this property being inversely proportional to the nanotube diameter. Recent work at GE Global Research has shown where a single nanotube device can behave as an "ideal" pn diode (5). The SWNT was bridged over a SiO2 channel between Mo contacts and exhibited an ideality factor of 1, based on a fit of the current-voltage data using the diode equation. The measured PV efficiency under a 0.8 eV monochromatic illumination showed a power conversion efficiency of 0.2 %. However, the projected efficiency of these junctions is estimated to be > 5 %, especially when one considers the enhanced absorption (from nanotubes whose bandgap is tailored to illumination) and electromagnetic coupling in a network of nanotubes.
Document ID
20090022304
Acquisition Source
Glenn Research Center
Document Type
Conference Paper
Authors
Efstathiadis, Harry
(Albany Univ. Albany, NY, United States)
Haldar, Pradeep
(Albany Univ. Albany, NY, United States)
Landi, Brian J.
(Rochester Inst. of Tech. NY, United States)
Denno, Patrick L.
(Rochester Inst. of Tech. NY, United States)
DiLeo, Roberta A.
(Rochester Inst. of Tech. NY, United States)
VanDerveer, William
(Rochester Inst. of Tech. NY, United States)
Raffaelle, Ryne P.
(Rochester Inst. of Tech. NY, United States)
Date Acquired
August 24, 2013
Publication Date
February 1, 2007
Publication Information
Publication: Proceedings of the 19th Space Photovoltaic Research and Technology Conference
Subject Category
Space Sciences (General)
Funding Number(s)
CONTRACT_GRANT: NNC05GA14G
CONTRACT_GRANT: ECS-0233776
CONTRACT_GRANT: NCC3-956
CONTRACT_GRANT: NAG3-2828
Distribution Limits
Public
Copyright
Public Use Permitted.
No Preview Available