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Diameter dependence of thermoelectric power of semiconducting carbon nanotubes

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Author(s)
Hung, Nguyen T.
•
Nugraha, Ahmad R. T.
•
Hasdeo, Eddwi H.
•
Saito, Riichiro
•
Dresselhaus, Mildred
Date Issued
October 2015
Journal
Physical Review B
Publisher
American Physical Society
Citation
Hung, Nguyen T., Ahmad R. T. Nugraha, Eddwi H. Hasdeo, Mildred S. Dresselhaus, and Riichiro Saito. "Diameter dependence of thermoelectric power of semiconducting carbon nanotubes." Phys. Rev. B 92, 165426 (October 2015). © 2015 American Physical Society
Version
Final published version
Abstract
We calculate the thermoelectric power (or thermopower) of many semiconducting single wall carbon nanotubes (s-SWNTs) within a diameter range 0.5–1.5 nm by using the Boltzmann transport formalism combined with an extended tight-binding model. We find that the thermopower of s-SWNTs increases as the tube diameter decreases. For some s-SWNTs with diameters less than 0.6 nm, the thermopower can reach a value larger than 2000 μV/K at room temperature, which is about 6 to 10 times larger than that found in commonly used thermoelectric materials. The large thermopower values may be attributed to the one dimensionality of the nanotubes and to the presence of large band gaps of the small-diameter s-SWNTs. We derive an analytical formula to reproduce the numerical calculation of the thermopower and we find that the thermopower of a given s-SWNT is directly related with its band gap. The formula also explains the shape of the thermopower as a function of tube diameter, which looks similar to the shape of the so-called Kataura plot of the band gap dependence on tube diameter.
MIT Department
Massachusetts Institute of Technology. Department of Electrical Engineering and Computer Science
Massachusetts Institute of Technology. Department of Physics
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Article is made available in accordance with the publisher's policy and may be subject to US copyright law. Please refer to the publisher's site for terms of use.
Persistent DSpace Link
http://hdl.handle.net/1721.1/99401
DOI of Published Version
https://doi.org/10.1103/PhysRevB.92.165426
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