Springer Theses / Energetic Materials at Extreme Conditions
(Sprache: Englisch)
Nominated for a Springer prize, this thesis explores the effects of extreme conditions on energetic materials and characterises new polymorphs obtained at high pressures and/or temperatures. It includes a superb analysis of future research opportunities.
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Nominated for a Springer prize, this thesis explores the effects of extreme conditions on energetic materials and characterises new polymorphs obtained at high pressures and/or temperatures. It includes a superb analysis of future research opportunities.
Klappentext zu „Springer Theses / Energetic Materials at Extreme Conditions “
David I.A. Millar's thesis explores the effects of extreme conditions on energetic materials. His study identifies and structurally characterises new polymorphs obtained at high pressures and/or temperatures. The performance of energetic materials (pyrotechnics, propellants and explosives) can depend on a number of factors including sensitivity to detonation, detonation velocity, and chemical and thermal stability. Polymorphism and solid-state phase transitions may therefore have significant consequences for the performance and safety of energetic materials. In order to model the behaviour of these important materials effectively under operational conditions it is essential to obtain detailed structural information at a range of temperatures and pressures.Inhaltsverzeichnis zu „Springer Theses / Energetic Materials at Extreme Conditions “
Introduction.- Experimental Techniques.- Structural Studies of RDX.- High-Pressure Structural Studies of CL-20.- Structural Investigation of a Series of Inorganic Azides (Part 1).- Structural Investigation of a Series of Inorganic Azides (Part 2).- General Remarks.
Bibliographische Angaben
- Autor: David I.A. Millar
- 2016, Softcover reprint of the original 1st ed. 2012, XIV, 222 Seiten, Maße: 15,5 x 23,5 cm, Kartoniert (TB), Englisch
- Verlag: Springer, Berlin
- ISBN-10: 366252113X
- ISBN-13: 9783662521137
Sprache:
Englisch
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