Do All Carbonized Charcoals Have the Same Chemical Structure? 1. Implications of Thermogravimetry−Mass Spectrometry Measurements

Erika Mészáros, Emma Jakab, Gábor Várhegyi, Jared Bourke, Merilyn Manley-Harris, Teppei Nunoura,§ and Michael Jerry Antal, Jr.*§
Chemical Research Center, Institute of Materials and Environmental Chemistry, Hungarian Academy of Sciences, P.O. Box 17, Budapest, Hungary, The Department of Chemistry, University of Waikato, Private Bag 3105, Hamilton, New Zealand, and The Hawaii Natural Energy Institute, School of Ocean and Earth Science and Technology, University of Hawaii at Manoa, Honolulu, Hawaii 96822
Ind. Eng. Chem. Res., 2007, 46 (18), pp 5943–5953
DOI: 10.1021/ie0615842
Publication Date (Web): June 26, 2007
Copyright © 2007 American Chemical Society

Abstract

A half century ago, Rosalind Franklin identified two distinct families of organic materials: those that become graphitic during carbonization at high temperatures and those that do not. According to Franklin, sucrose-derived biocarbons showed “no trace of homogeneous development of the true graphitic structure, even after heating to 3000 °C” [Proc. R. Soc. A 1951, 209, 196-218]. Franklin concluded that “non-graphitizing” carbons (e.g., sucrose biocarbons) are typically formed from oxygen-rich or hydrogen-poor substances that develop a “strong system of cross-linking, which immobilizes the structure and unites the crystallites in a rigid mass”. In this work, we show that there is a spectrum of non-graphitizing biocarbons ranging from those that release little CO during carbonization at temperatures approaching 1000 °C to those that strongly and persistently emit CO during carbonization at temperatures approaching 1000 °C. Typically, very low-ash biocarbons are not persistent CO emitters, but biocarbons with moderate ash contents can also be a member of this class if their ash lacks the catalytic species K, P, Mg, and/or Na that appear to be responsible for persistent CO evolution at 1000 °C.

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History

  • Published In Issue August 29, 2007
  • Received for review December 8, 2006
    Revised manuscript received May 1, 2007
    Accepted May 11, 2007

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