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Relationship Between Radiation Stability and Molecular Structure of Nitramine Explosives

Published online by Cambridge University Press:  15 February 2011

James J. Pinto
James J. Pinto*
Affiliation:
U. S. Army Armament Research, Development and Engineering Center, Picatinny Arsenal, NJ 07806-5000.
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Abstract

The radiation stabilities of the nitramine explosives 1,4-dinitroglycolurile (DINGU), 1,4-dimethyl-2,5-dinitroglycolurile (DMD) and hexanitrohexaazaisowurtzitane (HNIW) have been determined using XPS. Samples were exposed to x-rays for times up to eight hours while photoelectron spectra were recorded in the carbon, oxygen, and nitrogen Is energy regions and mass spectra were recorded of gases evolved during the decomposition process. These data are compared to the previously determined stabilities for cyclotrimethylene trinitramine (RDX) and cyclotetramethylene tetranitramine (HlMX). The N1s spectra of the irradiated materials show the NO2 peak decreases relative to the total nitrogen signal while low binding energy peaks grow. The rate of loss of the NO2 peak was fit to first order kinetics and the rate constants obtained show some correlation with the N-N bond strength as measured by the average N-N bond distance and the average NO2 asymetric stretch frequency. Despite the differences in structure of these molecules (DINGU and DMD are bicyclic rings, RDX and HMX are rings and HNIW is a cage) the radiation stability appears to be controlled by the strength of the N-N bond.

Type
Research Article
Information
MRS Online Proceedings Library (OPL) , Volume 296: Symposium Y – Structure and Properties of Energetic Materials , 1992 , 41
Copyright
Copyright © Materials Research Society 1993

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References

1. Brill, T. B. and Oyumi, Y., J. Phys. Chem., 90 (1986) 2679.Google Scholar
2. Owens, F., J. Mol. Struct. (THEOCHEM), 121 (1985) 213.Google Scholar
3. Murray, J. S. and Politzer, P., in Chemistry and Physics of Energetic Materials, edited by Bulusu, S. N. (Kluwer Academic Publishers, Dordrecht, the Netherlands, 1990) 157–173, and references therein.CrossRefGoogle Scholar
4. Wang, P. S. and Wittberg, T. N., J. Energet. Mat., 2 (1984) 167.Google Scholar
5. Beard, B. C. and Sharma, J., J. Energet. Mat., 7 (1989) 181.Google Scholar
6. Beard, B. C., Propellants, Explosives and Pyrotechnics, 16 (1991) 81.Google Scholar
7. Harris, J. (private communication).Google Scholar
8. Oyumi, Y. and Brill, T. B., Propellants, Explosives and Pyrotechnics, 13 (1988) 69.Google Scholar
9. Choi, C. S. and Prince, E., Acta Cryst., B28 (1972) 2857.CrossRefGoogle Scholar
10. Choi, C. S. and Boutin, H. P., Acta Cryst., B26 (1970) 1235.Google Scholar
11. Boileau, J., Wimmer, E., Gilardi, R., Stinecipher, M. M., Gallo, R. and Pirrrot, M., Acta Cryst., C44, (1988) 696.Google Scholar