Bis[3-(5-nitroimino-1,2,4-triazolate)]-Based Energetic Salts: Synthesis and Promising Properties of a New Family of High-Density Insensitive Materials

2010 ◽  
Vol 132 (34) ◽  
pp. 11904-11905 ◽  
Author(s):  
Ruihu Wang ◽  
Hongyan Xu ◽  
Yong Guo ◽  
Rongjian Sa ◽  
Jean’ne M. Shreeve
2017 ◽  
Vol 5 (30) ◽  
pp. 15525-15528 ◽  
Author(s):  
Xingye Li ◽  
Chenbin Wang ◽  
Haibo Li ◽  
Fude Nie ◽  
Hongquan Yin ◽  
...  

A new family of bishydrobis(tetrazol-1-yl)borate (BTB) based energetic ionic liquids were synthesized, which are hypergolic with oxidizers and show superior energy capacity and high density.


2020 ◽  
Vol 20 (2) ◽  
pp. 755-764 ◽  
Author(s):  
Ivan Gospodinov ◽  
Kostiantyn V. Domasevitch ◽  
Cornelia C. Unger ◽  
Thomas M. Klapötke ◽  
Jörg Stierstorfer

Author(s):  
A. Mocquet ◽  
O. Grasset ◽  
C. Sotin

Data extracted from the Extrasolar Planets Encyclo- paedia (see http://exoplanet.eu ) show the existence of planets that are more massive than iron cores that would have the same size. After meticulous verification of the data, we conclude that the mass of the smallest of these planets is actually not known. However, the three largest planets, Kepler-52b, Kepler-52c and Kepler-57b, which are between 30 and 100 times the mass of the Earth, have indeed density larger than an iron planet of the same size. This observation triggers this study that investigates under which conditions these planets could represent the naked cores of gas giants that would have lost their atmospheres during their migration towards the star. This study shows that for moderate viscosity values (10 25  Pa s or lower), large values of escape rate and associated unloading stress rate during the atmospheric loss process lead to the explosion of extremely massive planets. However, for moderate escape rate, the bulk viscosity and finite-strain incompressibility of the cores of giant planets can be large enough to retain a very high density during geological time scales. This would make those a new kind of planet, which would help in understanding the interior structure of the gas giants. However, this new family of exoplanets adds some degeneracy for characterizing terrestrial exoplanets.


2015 ◽  
Vol 39 (2) ◽  
pp. 893-901 ◽  
Author(s):  
Bo Wu ◽  
Zhixin Wang ◽  
Hongwei Yang ◽  
Qiuhan Lin ◽  
Xuehai Ju ◽  
...  

A series of energetic salts based on a guanidinium cation containing a picryl moiety was successfully synthesized and characterized.


RSC Advances ◽  
2015 ◽  
Vol 5 (27) ◽  
pp. 21422-21429 ◽  
Author(s):  
Hui Li ◽  
Feng-qi Zhao ◽  
Bo-zhou Wang ◽  
Lian-jie Zhai ◽  
Wei-peng Lai ◽  
...  

Dinitromethyl-functionalized energetic salts with acceptable oxygen balance and high detonation properties were reported.


2013 ◽  
Vol 1 (23) ◽  
pp. 6776 ◽  
Author(s):  
Qiu-Han Lin ◽  
Yu-Chuan Li ◽  
Cai Qi ◽  
Wei Liu ◽  
Yuan Wang ◽  
...  

2019 ◽  
Vol 43 (28) ◽  
pp. 11157-11163 ◽  
Author(s):  
Minxian Xu ◽  
Guangbin Cheng ◽  
Hualin Xiong ◽  
Bohan Wang ◽  
Xuehai Ju ◽  
...  

A new family of symmetric nitropyrazole and 1,2,4-triazole derivatives and its energetic salts were obtained. The positive effect of ternary hydrogen bonds improve the performances of target compounds.


2017 ◽  
Vol 2017 (1) ◽  
pp. 000689-000693
Author(s):  
Venky Sundaram ◽  
Fuhan Liu ◽  
Chandra Nair ◽  
Rao Tummala ◽  
Atsushi Kubo ◽  
...  

Abstract This paper presents the first demonstration of fine pitch embedded trench RDL on glass substrates using a new family of ultra-high resolution dry film photo-sensitive polymer dielectrics and a new large area panel scale lithography tool. The specific research targets are to demonstrate multilayer RDL scaling to 1um lines and vias at >200 I/Os per mm of die edge for 2.5D interposers and high density fan-out packages.


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