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101.
Characteristics and role of Al oxide (Al-O) films used as catalyst-support layer for vertical growth of single-walled carbon nanotubes (SWCNTs) were studied. EB-deposited Al films (20 nm) were thermally oxidized at 400 °C (10 min, static air) to produce the most appropriate surface structure of Al-O. Al-O catalyst-support layers were characterized using various analytical measurements, i.e., atomic force microscopy (AFM), X-ray photoelectron spectroscopy (XPS), and spectroscopy ellipsometry (SE). The thermally oxidized Al-O has a highly roughened surface, and also has the most suitable surface chemical states compared to other type of Al-O support layers. We suggest that the surface of thermally oxidized Al-O characterized in this work enhanced Co catalyst activity to promote the vertically aligned SWCNT growth. 相似文献
102.
We analyze the role of the electromagnetic field for the stability of a shearing viscous star with spherical symmetry. Matching conditions are given for the interior and the exterior metrics. We use a perturbation scheme to construct the collapse equation. The range of instability is explored in Newtonian and post Newtonian (pN) limits. We conclude that the electromagnetic field diminishes the effects of the shearing viscosity in the instability range and makes the system more unstable in both Newtonian and post Newtonian approximations. 相似文献
103.
The emission spectrum of SeO in the far ultraviolet first observed by Haranath (1) at low dispersion has been photographed in the region 2480-1930 Å under medium resolution and a reanalysis of the vibrational structure of the bands has been presented. Beginning at the longer wavelength end, the spectrum has been analyzed into five band systems which are designated as , x2-x1, y2-y1, , and . The lower state of the c-b system is found to be the upper state of the system observed recently by us (2). The derived constants in cm?1 for SeO are as follows (the constants of the b state are those derived from Ref. 2).
State | λ | |||
974 | 6.0 | |||
906 | 21.0 | |||
993 | 2.0 | |||
877 | 8.0 | |||
53080 | 954 | 13.0 | ||
51422 | 955 | 9.3 | ||
F1 | 51356 | 955 | 8.5 | ~36 |
50873 | 1034 | 9.3 | ||
9570.7 | 834.9 | 5.5 |