Abstract
Carbon fibers are unique reinforcing agents for lightweight composite materials due to their outstanding mechanical properties and low density. Current technologies are capable of producing carbon fibers with 90-95% of the modulus of perfect graphite (∼1025 GPa). However, these same carbon fibers possess less than 10% of the theoretical carbon fiber strength, estimated to be about 100 GPa. Traditionally, attempts to increase carbon fiber rigidity above a certain level results in lower breaking strength. Therefore, to develop advanced carbon fibers with both very high strength and modulus demands a new manufacturing methodology. Here, we report a method of manufacturing moderate strength, very high modulus carbon fibers from a very high molecular weight (VHMW) polyacrylonitrile (PAN) precursor without the use of nanomaterial additives such as nucleating or structure-templating agents, as have been used by others.
Original language | English |
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Pages (from-to) | 245-252 |
Number of pages | 8 |
Journal | Carbon |
Volume | 101 |
DOIs | |
State | Published - 2016 |
Funding
The authors would like to acknowledge financial support from DARPA . UKY authors (EAM and MCW) acknowledge financial support by Oak Ridge National Laboratory U.S. Department of Energy under award number 400095449 and 4000100727 . Electron microscopy work was supported by ORNL 's Shared Research Equipment (SHaRE) User Facility, which is sponsored by the Office of Basic Energy Sciences, US Department of Energy . Authors sincerely acknowledge help from Dr. Karren More (ORNL) with TEM characterization. SJM acknowledges additional support for equipment by NSF-MRI grant award number 1126534 and NSF-DMR grant award number 1006630 at Virginia Tech for molecular weight analysis and synthesis, respectively. The views, opinions, and/or findings contained in this paper are those of the authors and should not be interpreted as representing the official views or policies of the Department of Defense or the U.S. Government. This document is approved for Public Release, Distribution Unlimited. Notice: This manuscript has been authored by UT-Battelle, LLC under Contract No. DE-AC05-00OR22725 with the U.S. Department of Energy. The United States Government retains and the publisher, by accepting the article for publication, acknowledges that the United States Government retains a non-exclusive, paid-up, irrevocable, world-wide license to publish or reproduce the published form of this manuscript, or allow others to do so, for United States Government purposes. The Department of Energy will provide public access to these results of federally sponsored research in accordance with the DOE Public Access Plan ( http://energy.gov/downloads/doe-public-access-plan ).
Funders | Funder number |
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NSF-DMR | 1006630 |
NSF-MRI | |
Oak Ridge National Laboratory | 4000100727, 400095449 |
U.S. Department of Energy | |
Directorate for Mathematical and Physical Sciences | 1126534 |
Defense Advanced Research Projects Agency | |
Basic Energy Sciences | |
Oak Ridge National Laboratory |