DFT Study on the Impact of the Methylaluminoxane Cocatalyst in Ethylene Oligomerization Using a Titanium-Based Catalyst

2015 ◽  
Vol 34 (2) ◽  
pp. 426-431 ◽  
Author(s):  
Farhan Ahmad Pasha ◽  
Jean-Marie Basset ◽  
Hervé Toulhoat ◽  
Theodorus de Bruin
2018 ◽  
Vol 19 (2) ◽  
pp. 756-767 ◽  
Author(s):  
Xiao Zhao ◽  
Shiliang Huang ◽  
Yu Liu ◽  
Jinshan Li ◽  
Weihua Zhu

2013 ◽  
Vol 366 ◽  
pp. 238-246 ◽  
Author(s):  
Kamlesh N. Tayade ◽  
Manoj V. Mane ◽  
Suman Sen ◽  
C.N. Murthy ◽  
Gopal L. Tembe ◽  
...  

Author(s):  
Jun Zhang ◽  
Zhichao Wang ◽  
Lin Liu ◽  
Xufeng Ma ◽  
Yao Liu ◽  
...  

A two-carbon bridged diphosphine (PCCP) ligand bearing an ortho-methoxy substituent in the phosphine phenyl group has been synthesised and applied in Cr-catalysed ethylene tri-/tetramerization. Compared to previous catalysts, the Cr...


1962 ◽  
Vol 14 ◽  
pp. 415-418
Author(s):  
K. P. Stanyukovich ◽  
V. A. Bronshten

The phenomena accompanying the impact of large meteorites on the surface of the Moon or of the Earth can be examined on the basis of the theory of explosive phenomena if we assume that, instead of an exploding meteorite moving inside the rock, we have an explosive charge (equivalent in energy), situated at a certain distance under the surface.


1962 ◽  
Vol 14 ◽  
pp. 169-257 ◽  
Author(s):  
J. Green

The term geo-sciences has been used here to include the disciplines geology, geophysics and geochemistry. However, in order to apply geophysics and geochemistry effectively one must begin with a geological model. Therefore, the science of geology should be used as the basis for lunar exploration. From an astronomical point of view, a lunar terrain heavily impacted with meteors appears the more reasonable; although from a geological standpoint, volcanism seems the more probable mechanism. A surface liberally marked with volcanic features has been advocated by such geologists as Bülow, Dana, Suess, von Wolff, Shaler, Spurr, and Kuno. In this paper, both the impact and volcanic hypotheses are considered in the application of the geo-sciences to manned lunar exploration. However, more emphasis is placed on the volcanic, or more correctly the defluidization, hypothesis to account for lunar surface features.


1997 ◽  
Vol 161 ◽  
pp. 197-201 ◽  
Author(s):  
Duncan Steel

AbstractWhilst lithopanspermia depends upon massive impacts occurring at a speed above some limit, the intact delivery of organic chemicals or other volatiles to a planet requires the impact speed to be below some other limit such that a significant fraction of that material escapes destruction. Thus the two opposite ends of the impact speed distributions are the regions of interest in the bioastronomical context, whereas much modelling work on impacts delivers, or makes use of, only the mean speed. Here the probability distributions of impact speeds upon Mars are calculated for (i) the orbital distribution of known asteroids; and (ii) the expected distribution of near-parabolic cometary orbits. It is found that cometary impacts are far more likely to eject rocks from Mars (over 99 percent of the cometary impacts are at speeds above 20 km/sec, but at most 5 percent of the asteroidal impacts); paradoxically, the objects impacting at speeds low enough to make organic/volatile survival possible (the asteroids) are those which are depleted in such species.


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