Theoretical investigations of ozone vibrational relaxation and oxygen atom diffusion rates in Ar and xenon matrixes

1993 ◽  
Vol 97 (47) ◽  
pp. 12134-12143 ◽  
Author(s):  
M. Beth Ford ◽  
Angel D. Foxworthy ◽  
G. J. Mains ◽  
Lionel M. Raff
1994 ◽  
Vol 98 (51) ◽  
pp. 13766-13771 ◽  
Author(s):  
Martin D. Perry ◽  
Gilbert J. Mains ◽  
Lionel M. Raff

2015 ◽  
Vol 579 ◽  
pp. 123-126 ◽  
Author(s):  
Shao-Long Jiang ◽  
Xi Chen ◽  
Jing-Yan Zhang ◽  
Guang Yang ◽  
Jiao Teng ◽  
...  
Keyword(s):  

1996 ◽  
Vol 53 (12) ◽  
pp. 7731-7735 ◽  
Author(s):  
T. Brudevoll ◽  
E. A. Kotomin ◽  
N. E. Christensen

2014 ◽  
Vol 168 ◽  
pp. 151-166 ◽  
Author(s):  
Emanuele Congiu ◽  
Marco Minissale ◽  
Saoud Baouche ◽  
Henda Chaabouni ◽  
Audrey Moudens ◽  
...  

At the low temperatures of interstellar dust grains, it is well established that surface chemistry proceeds via diffusive mechanisms of H atoms weakly bound (physisorbed) to the surface. Until recently, however, it was unknown whether atoms heavier than hydrogen could diffuse rapidly enough on interstellar grains to react with other accreted species. In addition, models still require simple reduction as well as oxidation reactions to occur on grains to explain the abundances of various molecules. In this paper we investigate O-atom diffusion and reactivity on a variety of astrophysically relevant surfaces (water ice of three different morphologies, silicate, and graphite) in the 6.5–25 K temperature range. Experimental values were used to derive a diffusion law that emphasizes that O atoms diffuse by quantum mechanical tunnelling at temperatures as low as 6.5 K. The rates of diffusion on each surface, based on modelling results, were calculated and an empirical law is given as a function of the surface temperature. The relative diffusion rates are kH2Oice > ksil > kgraph ≫ kexpected. The implications of efficient O-atom diffusion over astrophysically relevant time-scales are discussed. Our findings show that O atoms can scan any available reaction partners (e.g., either another H atom, if available, or a surface radical like O or OH) at a faster rate than that of accretion. Also, as dense clouds mature, H2 becomes far more abundant than H and the O : H ratio grows, and the reactivity of O atoms on grains is such that O becomes one of the dominant reactive partners together with H.


2005 ◽  
Vol 8 (3) ◽  
pp. 239-243 ◽  
Author(s):  
Luciano Henrique de Almeida ◽  
Kelly Cristina Cezaretto Pires ◽  
Carlos Roberto Grandini ◽  
Odila Florêncio
Keyword(s):  

Author(s):  
G.J.C. Carpenter

In zirconium-hydrogen alloys, rapid cooling from an elevated temperature causes precipitation of the face-centred tetragonal (fct) phase, γZrH, in the form of needles, parallel to the close-packed <1120>zr directions (1). With low hydrogen concentrations, the hydride solvus is sufficiently low that zirconium atom diffusion cannot occur. For example, with 6 μg/g hydrogen, the solvus temperature is approximately 370 K (2), at which only the hydrogen diffuses readily. Shears are therefore necessary to produce the crystallographic transformation from hexagonal close-packed (hep) zirconium to fct hydride.The simplest mechanism for the transformation is the passage of Shockley partial dislocations having Burgers vectors (b) of the type 1/3<0110> on every second (0001)Zr plane. If the partial dislocations are in the form of loops with the same b, the crosssection of a hydride precipitate will be as shown in fig.1. A consequence of this type of transformation is that a cumulative shear, S, is produced that leads to a strain field in the surrounding zirconium matrix, as illustrated in fig.2a.


Author(s):  
P.A. Midgley ◽  
R. Vincent ◽  
D. Cherns

The oxygenation of YBa2Cu3O7−x (YBCO) leads to an orthorhombic distortion of the unit cell to accommodate the extra oxygen atom. This makes the formation of twins energetically favourable with CuO4 planar unit chains running alternately along the a and b axes of the parent tetragonal structure. The geometry of this twinning is such that four possible twin variants may co-exist with the twin boundaries lying in the (110) or (110) planes of the deformed structure. The traces of these planes are not mutually perpendicular and thus the crystal is strained to allow for the mismatch. It is to the nature of this strain field that this work has been addressed.Sintered samples were prepared by crushing and dispersing the resultant powder onto a very fine Cu mesh grid. Single crystals were chemically thinned to perforation. No discernible artefacts were seen and similar results were obtained with either method.


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