Published December 23, 2003 | Version Published
Book Section - Chapter Open

Field emission testing of carbon nanotubes for THz frequency vacuum microtube sources

  • 1. ROR icon Jet Propulsion Lab
  • 2. ROR icon California Institute of Technology

Abstract

A carbon nanotube-based high current density electron field emission source is under development at Jet Propulsion Laboratory (JPL) for submillimeter-wave power generation (300 GHz to 3 THz). This source is the basis for a novel vacuum microtube component: the nanoklystron. The nanoklystron is a monolithically fabricated reflex klystron with dimensions in the micrometer range. The goal is to operate this device at much lower voltages than would be required with hot-electron sources and at much higher frequencies than have ever been demonstrated. Both single-walled (SWNTs) as well as multi-walled nanotubes (MWNTs) are being tested as potential field-emission sources. This paper presents initial results and observations of these field emission tests. SWNTs and MWNTs were fabricated using standard CVD techniques. The tube density was higher in the case of MWNT samples. As previously reported, high-density samples suffered from enhanced screening effect thus decreasing their total electron emission. The highest emission currents were measured from disordered, less dense MWNTs and were found to be ~0.63 mA @ 3.6 V/μm (sample 1) and ~3.55 mA @ 6.25 V/μm (sample 2). The high density vertically aligned MWNTs showed low field emission as predicted: 0.31 mA @ 4.7 V/μm.

Additional Information

© 2003 Society of Photo-Optical Instrumentation Engineers (SPIE). This research was carried out at the Jet Propulsion Laboratory, California Institute of Technology, under a contract with National Aeronautics and Space Administration (NASA). This work was funded by NASA's Code-R grants and JPL's Director's Research and Development Fund. Authors would like to thank Colleen Marrese of JPL and Dr. James Hone of California Institute of Technology (currently at Columbia University) for their initial help.

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Identifiers

Eprint ID
87690
Resolver ID
CaltechAUTHORS:20180710-095629084

Funding

NASA/JPL/Caltech
JPL Director's Research and Development Fund

Dates

Created
2018-07-10
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Updated
2021-11-15
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Caltech Custom Metadata

Caltech groups
Physics Department
Series Name
Proceedings of SPIE
Series Volume or Issue Number
5343