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Magnetic and Magneto-Optical Properties of Co-Sputtering FePt Films
J. Gao,B. Ma,C.L. Zha,Q.Y. Jin,S.Y. Wang,Z.Z. Zhang 한국물리학회 2006 THE JOURNAL OF THE KOREAN PHYSICAL SOCIETY Vol.49 No.5I
FePt thin .lms have been prepared at dierent substrate temperatures by DC magnetron co-sputtering. The .lms change from a disordered fcc structure to a L10 fct structure with temperature. The magnetic and the magneto-optical properties of those FePt .lms have been studied. The dependence of spectral changes on the formation of a chemically-ordered L10structure is observed in the polar magneto-optical Kerr rotation. In the spectra, the ultraviolet peak located in the high-energy range (4.0 { 4.5 eV), which is related to electronic transitions on Pt atomic sites, is observed for all samples. On the contrary, the peak related to transitions on Fe atomic sites, which is located in the low-energy range (1.5 { 2.0 eV), is only observed for highly chemically-ordered samples. Compared with the spectra for the L10 structure of FePt .lms pre- pared by using molecular beam epitaxy, the infrared peak related to Fe sites is shifted to low energy.
L. Cheng,S.M. Zhang,P.P. Chen,S.L. Huang,L. Liu,W. Zhou,J. Liu,H. Gong,Q.M. Luo 한국물리학회 2007 Current Applied Physics Vol.7 No.s1
Poly(D,L-lactide) (PDLLA)/uorohydroxyapatite nanocrystals (nano-F-HA) porous scaolds were successfully fabricated through asolvent-casting and particulate-leaching technique. Nano-HA/PDLLA scaold and PDLLA scaold were prepared by using the sameprocess for comparison. The structure, phase and morphology of the nanocomposite scaolds were observed by SEM. The results indi-cated that F-HA nanocrystals were homogeneously dispersed in the PDLLA matrix. The porosity of the scaolds was up to 90%, andmacropores and micropores coexisted and interconnected throughout the scaolds. Cell culture experiments demonstrated that the nano-F-HA/PDLLA scaffold had the best adhesion tendency to chondrocytes among the scaffolds investigated.
Li, C.J.,Xu, Z.H.,Dong, Z.X.,Shi, S.L.,Zhang, J.G. Asian Australasian Association of Animal Productio 2016 Animal Bioscience Vol.29 No.8
Whole-crop wheat (Triticum aestivum L.) as forage has been extensively used in the world. In this study, the effects of N application rates on the yields, nutritive value and silage quality were investigated. The N application rates were 0, 75, 150, 225, and 300 kg/ha. The research results indicated that the dry matter yield of whole-crop wheat increased significantly with increasing N rate up to 150 kg/ha, and then leveled off. The crude protein content and in vitro dry matter digestibility of whole-crop wheat increased significantly with increasing N up to 225 kg/ha, while they no longer increased at N 300 kg/ha. On the contrary, the content of various fibers tended to decrease with the increase of N application. The content of lactic acid, acetic acid and propionic acid in silages increased with the increase of N rate (p<0.05). The ammonia-N content of silages with higher N application rates (${\geq}225kg/ha$) was significantly higher than that with lower N application rates (${\leq}150kg/ha$). Whole-crop wheat applied with high levels of N accumulated more nitrate-N. In conclusion, taking account of yields, nutritive value, silage quality and safety, the optimum N application to whole-crop wheat should be about 150 kg/ha at the present experiment conditions.
Effects of Maturity Stages on the Nutritive Composition and Silage Quality of Whole Crop Wheat
Xie, Z.L.,Zhang, T.F.,Chen, X.Z.,Li, G.D.,Zhang, J.G. Asian Australasian Association of Animal Productio 2012 Animal Bioscience Vol.25 No.10
The changes in yields and nutritive composition of whole crop wheat (Triticum aestivum L.) during maturation and effects of maturity stage and lactic acid bacteria (LAB) inoculants on the fermentation quality and aerobic stability were investigated under laboratory conditions. Whole crop wheat harvested at three maturation stages: flowering stage, milk stage and dough stage. Two strains of LAB (Lactobacillus plantarum: LAB1, Lactobacillus parafarraqinis: LAB2) were inoculated for wheat ensiling at $1.0{\times}10^5$ colony forming units per gram of fresh forage. The results indicated that wheat had higher dry matter yields at the milk and dough stages. The highest water-soluble carbohydrates content, crude protein yields and relative feed value of wheat were obtained at the milk stage, while contents of crude fiber, neutral detergent fiber and acid detergent fiber were the lowest, compared to the flowering and dough stages. Lactic acid contents of wheat silage significantly decreased with maturity. Inoculating homofermentative LAB1 markedly reduced pH values and ammonia-nitrogen ($NH_3$-N) content (p<0.05) of silages at three maturity stages compared with their corresponding controls. Inoculating heterofermentative LAB2 did not significantly influence pH values, whereas it notably lowered lactic acid and $NH_3$-N content (p<0.05) and effectively improved the aerobic stability of silages. In conclusion, considering both yields and nutritive value, whole crop wheat as forage should be harvested at the milk stage. Inoculating LAB1 improved the fermentation quality, while inoculating LAB2 enhanced the aerobic stability of wheat silages at different maturity stages.
Sensitivity of surface characteristics on the simulation of wind-blown-dust source in North America
Park, S.H.,Gong, S.L.,Gong, W.,Makar, P.A.,Moran, M.D.,Stroud, C.A.,Zhang, J. Pergamon Press ; Elsevier [distribution] 2009 Atmospheric environment Vol.43 No.19
Recently, a wind-blown-dust-emission module has been built based on a state-of-the-art wind erosion theory and evaluated in a regional air-quality model to simulate a North American dust storm episode in April 2001 (see Park, S.H., Gong, S.L., Zhao, T.L., Vet, R.J., Bouchet, V.S., Gong, W., Makar, P.A., Moran, M.D., Stroud, C., Zhang, J. 2007. Simulation of entrainment and transport of dust particles within North America in April 2001 (''Red Dust episode''). J. Geophys. Res. 112, D20209, doi:10.1029/2007JD008443). A satisfactorily detailed assessment of that module, however, was not possible because of a lack of information on some module inputs, especially soil moisture content. In this paper, the wind-blown-dust emission was evaluated for two additional dust storms using improved soil moisture inputs. The surface characteristics of the wind-blown-dust source areas in southwestern North America were also investigated, focusing on their implications for wind-blown-dust emissions. The improved soil moisture inputs enabled the sensitivity of other important surface characteristics, the soil grain size distribution and the land-cover, to dust emission to be investigated with more confidence. Simulations of the two 2003 dust storm episodes suggested that wind-blown-dust emissions from the desert areas in southwestern North America are dominated by emissions from dry playas covered with accumulated alluvial deposits whose particle size is much smaller than usual desert sands. As well, the source areas in the northwestern Texas region were indicated to be not desert but rather agricultural lands that were ''activated'' as a wind-blown-dust sources after harvest. This finding calls for revisions to the current wind-blown-dust-emission module, in which ''desert'' is designated to be the only land-cover category that can emit wind-blown dust.
Logarithmically completely monotonic functions and Gurland's ratio for the gamma function
Y. J. Wei,S. L. Zhang,C. P. Chen 장전수학회 2007 Advanced Studies in Contemporary Mathematics Vol.15 No.2
Two logarithmically completely monotonic functions involving gamma function are proved. As an application, bounds for the ratio T(x;y) = ( x)(y)= 2((x+y)=2) is established and the corresponding result by J. D. keckic and P. M.Vasic is refined.
Leakage Currents of a Fast Switching Thyristor Made by Proton Irradiation Method
E.D. Kim,C.L. Zhang,S.C. Kim,N.K. Kim,J.Z. Zhu,B.F. Yang 전력전자학회 2004 ICPE(ISPE)논문집 Vol.- No.-
A thyristor with a VRRM of 1,600V was made with 200μm of N-base width from 60Ω·cm NTD-Si wafer and the proton irradiation was employed for improving its switching performance. This study showed that 4.7MeV-proton irradiation gives a narrow distribution of induced defects in the middle of N-drift region with its width of 10μm, which resulted in a superior trade-off relation between its static and dynamic characteristics. It was found that 3.7MeV and 5.9MeV protons remarkably increased the forward leakage current IDRM and the reverse leakage current IRRM, respectively. The increased IDRM and IRRM are attributed to the induced defects in the depletion layers of thyristor junctions J2 and J1, respectively.
Relativistic jet activity from the tidal disruption of a star by a massive black hole
Burrows, D. N.,Kennea, J. A.,Ghisellini, G.,Mangano, V.,Zhang, B.,Page, K. L.,Eracleous, M.,Romano, P.,Sakamoto, T.,Falcone, A. D.,Osborne, J. P.,Campana, S.,Beardmore, A. P.,Breeveld, A. A.,Chester, Nature Publishing Group, a division of Macmillan P 2011 Nature Vol.476 No.7361
Supermassive black holes have powerful gravitational fields with strong gradients that can destroy stars that get too close, producing a bright flare in ultraviolet and X-ray spectral regions from stellar debris that forms an accretion disk around the black hole. The aftermath of this process may have been seen several times over the past two decades in the form of sparsely sampled, slowly fading emission from distant galaxies, but the onset of the stellar disruption event has not hitherto been observed. Here we report observations of a bright X-ray flare from the extragalactic transient Swift J164449.3+573451. This source increased in brightness in the X-ray band by a factor of at least 10,000 since 1990 and by a factor of at least 100 since early 2010. We conclude that we have captured the onset of relativistic jet activity from a supermassive black hole. A companion paper comes to similar conclusions on the basis of radio observations. This event is probably due to the tidal disruption of a star falling into a supermassive black hole, but the detailed behaviour differs from current theoretical models of such events.