scholarly journals H2 Formation on Interstellar Grains and the Fate of Reaction Energy

2021 ◽  
Vol 917 (1) ◽  
pp. 49
Author(s):  
Stefano Pantaleone ◽  
Joan Enrique-Romero ◽  
Cecilia Ceccarelli ◽  
Stefano Ferrero ◽  
Nadia Balucani ◽  
...  
1998 ◽  
Vol 296 (4) ◽  
pp. 869-872 ◽  
Author(s):  
O. Biham ◽  
I. Furman ◽  
N. Katz ◽  
V. Pirronello ◽  
G. Vidali

2000 ◽  
pp. 99-106 ◽  
Author(s):  
D. A. Williams ◽  
D. E. Williams ◽  
D. Clary ◽  
A. Farebrother ◽  
A. Fisher ◽  
...  

Nanomaterials ◽  
2021 ◽  
Vol 11 (4) ◽  
pp. 978
Author(s):  
Ming-Jie Zhao ◽  
Zhi-Xuan Zhang ◽  
Chia-Hsun Hsu ◽  
Xiao-Ying Zhang ◽  
Wan-Yu Wu ◽  
...  

Indium oxide (In2O3) film has excellent optical and electrical properties, which makes it useful for a multitude of applications. The preparation of In2O3 film via atomic layer deposition (ALD) method remains an issue as most of the available In-precursors are inactive and thermally unstable. In this work, In2O3 film was prepared by ALD using a remote O2 plasma as oxidant, which provides highly reactive oxygen radicals, and hence significantly enhancing the film growth. The substrate temperature that determines the adsorption state on the substrate and reaction energy of the precursor was investigated. At low substrate temperature (100–150 °C), the ratio of chemically adsorbed precursors is low, leading to a low growth rate and amorphous structure of the films. An amorphous-to-crystalline transition was observed at 150–200 °C. An ALD window with self-limiting reaction and a reasonable film growth rate was observed in the intermediate temperature range of 225–275 °C. At high substrate temperature (300–350 °C), the film growth rate further increases due to the decomposition of the precursors. The resulting film exhibits a rough surface which consists of coarse grains and obvious grain boundaries. The growth mode and properties of the In2O3 films prepared by plasma-enhanced ALD can be efficiently tuned by varying the substrate temperature.


Author(s):  
Di Li ◽  
Yingying Xing ◽  
Changjian Zhou ◽  
Yikai Lu ◽  
Shengjie Xu ◽  
...  

The high reaction energy barrier of the oxygen evolution reaction (OER) extremely reduces the efficiency of water splitting, which is not conducive to large-scale production of hydrogen. Due to the...


1987 ◽  
Vol 120 ◽  
pp. 167-169
Author(s):  
Valerio Pirronello

The problem of the formation of molecular hydrogen in interstellar clouds is revisited. the role played by cosmic ray bombardment under certain circumstances is considered mainly in the light of the low formation rate of H2 on grains due to the reduced mobility of adsorbed H atoms on their amorphous surfaces at interstellar temperatures.


1998 ◽  
Vol 63 (18) ◽  
pp. 6390-6393 ◽  
Author(s):  
Georgios Vassilikogiannakis ◽  
Manolis Stratakis ◽  
Michael Orfanopoulos

2000 ◽  
Vol 105 (A5) ◽  
pp. 10299-10302 ◽  
Author(s):  
A. N. Witt
Keyword(s):  

2017 ◽  
Vol 19 (15) ◽  
pp. 9798-9805 ◽  
Author(s):  
Johannes T. Margraf ◽  
Duminda S. Ranasinghe ◽  
Rodney J. Bartlett

We describe the automatic generation of reaction energy benchmark sets from arbitrary atomization energy reference data.


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