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In relation to this article, we declare that there is no conflict of interest.
Publication history
Received September 25, 2007
Accepted May 10, 2008
articles This is an Open-Access article distributed under the terms of the Creative Commons Attribution Non-Commercial License (http://creativecommons.org/licenses/bync/3.0) which permits unrestricted non-commercial use, distribution, and reproduction in any medium, provided the original work is properly cited.
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Photochemical reduction of molecular weight and number of double bonds in natural rubber film

Department of Chemical Technology, Faculty of Science, Chulalongkorn University, Bangkok, Thailand
wannipha@okuno-auromex.com
Korean Journal of Chemical Engineering, November 2008, 25(6), 1532-1538(7), 10.1007/s11814-008-0252-6
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Abstract

Abstract.Natural rubber (NR) can be degraded depending on various factors such as heat, mechanical force, chemical reaction, and light. Light is a very interesting factor because it can cause the NR to degrade under low temperature and pressure. The photo-degradation of NR films was carried out to investigate the effects of the light and the temperature on the reduction of the weight-average molecular weight (Mw) and the double bonds in the NR films. The NR films, with and without catalysts, titanium dioxide (TiO2), and potassium persulfate (K2S2O8), were exposed to light from a mercury light bulb at 7,000 and 36,000 lux, and at the temperature of 25 ℃ and 80 ℃ for 192 hrs. After exposure, the Mw of the NR films was analyzed by gel permeation chromatography (GPC). Changes in the Mw were used to construct a kinetic model for the process, (1/Mw)=(1/Mw0)+(kt/2M0) where k is the rate constant, and M0 is the Mw of the monomer unit. The linear relationship between 1/Mw and time suggested pseudo first-order processes with random scission. The Mw distribution information from the GPC was used to calculate the number of double bonds in the NR films. The trend of the double bonds reduction curves was quite similar to the result obtained from the calculation from the FTIR spectra. This indicated that this calculation method might possibly be another alternative way to obtain the_x000D_ number of double bonds in the NR.

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