980 resultados para Triton X-114
Resumo:
We study the diffuse X-ray luminosity (L-X) of star-forming galaxies using two-dimensional axisymmetric hydrodynamical simulations and analytical considerations of supernovae-(SNe-) driven galactic outflows. We find that the mass loading of the outflows, a crucial parameter for determining the X-ray luminosity, is constrained by the availability of gas in the central star-forming region, and a competition between cooling and expansion. We show that the allowed range of the mass loading factor can explain the observed scaling of L-X with star formation rate (SFR) as L-X alpha SFR2 for SFR greater than or similar to 1 M-circle dot yr(-1), and a flatter relation at low SFRs. We also show that the emission from the hot circumgalactic medium (CGM) in the halo of massive galaxies can explain the large scatter in the L-X-SFR relation for low SFRs (less than or similar to few M-circle dot yr(-1)). Our results suggest that galaxies with small SFRs and large diffuse X-ray luminosities are excellent candidates for the detection of the elusive CGM.
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Cu2SnS3 thins films were deposited onto In2O3: Sn coated soda lime glass substrates by spin coating technique. The films have been structurally characterized using x-ray Diffraction (XRD) and Atomic Force Microscopy (AFM). The morphology of the films was studied using Field Emission Scanning Electron Microscopy (FESEM). The optical properties of the films were determined using UV-vis-NIR spectrophotometer. The electrical properties were measured using Hall effect measurements. The energy band offsets at the Cu2SnS3/In2O3: Sn interface were calculated using x-ray photoelectron spectroscopy (XPS). The valence band offset was found to be -3.4 +/- 0.24 eV. From the valence band offset value, the conduction band offset is calculated to be -1.95 +/- 0.34 eV. The energy band alignment indicates a type-II misaligned heterostructure formation.
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We report the transition from robust ferromagnetism to a spin- glass state in nanoparticulate La0.7Sr0.3MnO3 through solid solution with BaTiO3. The field- and temperature-dependent magnetization and the frequency-dependent ac magnetic susceptibility measurements strongly indicate the existence of a spin- glass state in the system, which is further confirmed from memory effect measurements. The breaking of long-range ordering into short-range magnetic domains is further investigated using density-functional calculations. We show that Ti ions remain magnetically inactive due to insufficient electron leakage from La0.7Sr0.3MnO3 to the otherwise unoccupied Ti-d states. This results in the absence of a Mn-Ti-Mn spin exchange interaction and hence the breaking of the long-range ordering. Total-energy calculations suggest that the segregation of nonmagnetic Ti ions leads to the formation of short-range ferromagnetic Mn domains.
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We report the localized charge carrier transport of two-phase composite Zn1-x Ni (x) O/NiO (0 a parts per thousand currency sign x a parts per thousand currency sign 1) using the temperature dependence of ac-resistivity rho (ac)(T) across the N,el temperature T (N) (= 523 K) of nickel oxide. Our results provide strong evidence to the variable range hopping of charge carriers between the localized states through a mechanism involving spin-dependent activation energies. The temperature variation of carrier hopping energy epsilon (h)(T) and nearest-neighbor exchange-coupling parameter J (ij)(T) evaluated from the small poleron model exhibits a well-defined anomaly across T (N). For all the composite systems, the average exchange-coupling parameter (J (ij))(AVG) nearly equals to 70 meV which is slightly greater than the 60-meV exciton binding energy of pure zinc oxide. The magnitudes of epsilon (h) (similar to 0.17 eV) and J (ij) (similar to 11 meV) of pure NiO synthesized under oxygen-rich conditions are consistent with the previously reported theoretical estimation based on Green's function analysis. A systematic correlation between the oxygen stoichiometry and, epsilon (h)(T) and J (ij)(T) is discussed.
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Exploring future cathode materials for sodium-ion batteries, alluaudite class of Na2Fe2II(SO4)(3) has been recently unveiled as a 3.8 V positive insertion candidate (Barpanda et al. Nat. Commun. 2014, 5, 4358). It forms an Fe-based polyanionic compound delivering the highest Fe-redox potential along with excellent rate kinetics and reversibility. However, like all known SO4-based insertion materials, its synthesis is cumbersome that warrants careful processing avoiding any aqueous exposure. Here, an alternate low temperature ionothermal synthesis has been described to produce the alluaudite Na2+2xFe2-xII(SO4)(3). It marks the first demonstration of solvothermal synthesis of alluaudite Na2+2xM2-xII(SO4)(3) (M = 3d metals) family of cathodes. Unlike classical solid-state route, this solvothermal route favors sustainable synthesis of homogeneous nanostructured alluaudite products at only 300 degrees C, the lowest temperature value until date. The current work reports the synthetic aspects of pristine and modified ionothermal synthesis of Na2+2xFe2-xII(SO4)(3) having tunable size (300 nm similar to 5 mu m) and morphology. It shows antiferromagnetic ordering below 12 K. A reversible capacity in excess of 80 mAh/g was obtained with good rate kinetics and cycling stability over 50 cycles. Using a synergistic approach combining experimental and ab initio DFT analysis, the structural, magnetic, electronic, and electrochemical properties and the structural limitation to extract full capacity have been described.
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III-V pentenary semiconductor AlGaInPAs with a direct band gap of up to 2.0 eV has been grown successfully on GaAs substrates by liquid phase epitaxy;(LPE). With the introduction of the energy bowing parameters of quaternaries, the theoretical calculations agree well with the measured PL peak energy data from pentenary samples.
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The Ga1-xMnxSb samples were fabricated by the implantation of Mn ions into GaSb (1 0 0) substrate with mass-analyzed low-energy dual ion beam deposition system, and post-annealing. Auger electron spectroscopy depth profile of the Ga1-xMnxSb samples showed
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A new X-ray diffraction method for characterising thermal mismatch stress (TMS) in SiCw–Al composite has been developed. The TMS and thermal mismatch strain (TMSN) in SiC whiskers are considered to be axis symmetrical, and can be calculated by measuring the lattice distortion of the whiskers. Not only the average TMS in whiskers and matrix can be obtained, but the TMS components along longitudinal and radial directions in the SiC whiskers can also be deduced. Experimental results indicate that the TMS in SiC whiskers is compressive, and tensile in the aluminium matrix. The TMS and TMSN components along the longitudinal direction in the SiC whiskers are greater than those along the radial direction for a SiCw–Al composite quenched at 500°C.
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Con el propósito de determinar la producción de la biomasa forrajera y la concentración de nutrientes del pasto cubano CT - 115, se realizó un estudio en la Finca la Tigra, Cárdenas, Rivas, para ello se utilizó un área de 48 m2, subdividida en tres parcelas de 16 m2, donde se realizaron cortes a los 15, 30, 45, 60 y 75 días. Se evaluaron las variables altura de la planta, producción de biomasa fresca y seca por hectárea, en cada muestreo se tomaron muestras de plantas de 1,000 g, las que fueron remitidas al laboratorio de suelo y planta de la UNA, donde se hicieron las determinaciones de contenido de materia seca, % de nitrógeno, % fósforo, % potasio, % calcio, % magnesio, hierro (ppm), manganeso (ppm) y zinc (ppm). Se realizarón análisis de correlación usando el programa SAS (Sistema de Análisis Estadístico) versión 9. para los elementos de la composición nutritiva de la planta y las variables rendimiento de biomasa y altura, a través del programa CVEXPT (Experto de Curvas) versión 1.4, se determinaron las curvas de mejor ajustes para dichas relaciones. Encontrándose que a medida que aumentaba la edad de corte, la producción de biomasa fresca y seca así como la altura tendían a incrementar, inversamente a ello los niveles de nutrientes en las plantas, las ecuaciones de mejor ajustes para la producción de biomasa fresca, seca y altura fueron el Lineal, Logístico y Rotacional, con r2 de 94, 98 y 99% respectivamente, para el caso de los nutrientes las ecuaciones de mejor ajuste fueron: los modelos de función Rotacional, Logístico, Polinomial y Harris también con r2 de 92 a 99%, evidenciándose con esto que las tendencias de los incrementos de la biomasa seca, altura, y la concentración de nutrientes no presentan comportamiento lineal. Únicamente para el caso de la biomasa fresca se presentó una tendencia lineal.
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Con el objetivo de evaluar la Productividad y concentración de nutrientes del pasto cubano (Pennisetum purpureum x Pennisetum typhoides) cv CT – 115, se llevó a cabo la presente investigación en la finca Santa Rosa propiedad de la Universidad Nacional Agraria (UNA) Managua, Nicaragua. Localizada geográficamente a los 12° 08´ 33"de latitud norte y, 86° 10´ 31" de longitud oeste (INETER, 2006). Para ello se utilizó un área total de 33 m2 la cual se subdividió en tres parcelas de 10 m2 cada una donde se realizaron cortes cada 15 días hasta llegar a los 75 días. Se evaluaron las variables : altura, (cm) biomasa fresca (kg ha-1), Materia Seca (%), Biomasa seca (kg ha-1), Nitrógeno (%), Fósforo (%), Potasio (%),Calcio (%), Magnesio (%), Hierro (ppm), Manganeso (ppm), Zinc (ppm). Para la determinación de la producción de biomasa verde y seca (kg ha-1), se utilizó la metodología propuesta por la Red Internacional de evaluación de Pasturas Tropicales (CIAT, 1982). Para determinar los parámetros MS (%) se utilizó la metodología del análisis de Weende o análisis proximal (AOAC. 1990). Para el análisis de correlación se utilizo el programa SAS VERSION 9 para cada uno de las variables evaluadas, para la determinación de las curvas de mejor ajuste se utilizó el programa CVXP32. Durante el ensayo no se aplico ningún tipo de tratamiento agronómico (fertilización, riego). Los resultados obtenidos fueron: Altura 220 cm Biomasa fresca 31,764 kg ha-1 Materia seca 24% Biomasa seca 7529 kg ha-1. Las mayores concentraciones de nutrientes en la planta fueron: N 3.21% P 0.38% K 4.94% Ca 0.24% Mg 0.18% Fe 105.0ppm Mn 53.33ppm Zn 50ppm. Los modelos de mejor ajuste son: Modelo Múltiple Multiplicativo, Modelo Richards, Modelo Harris, Función Rotacional, Tercer Grado Polinomial y Asociación Exponencial.
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Bulk metallic glasses of Nd65Al10Fe25-xCox (x=0,5,10) have been prepared in the form of 3 mm diam rods. Results of differential scanning calrimetry, dynamic mechanical thermal analysis (DMTA), and x-ray diffraction are presented for these alloys. It is shown that the glass transition and crystallization have been observed by DMTA. The reduced glass transition temperature of these glasses, defined as the ratio between the glass transition temperature T-g and the melting temperature T-l is in the range from 0.55 to 0.62. All these glasses have a large supercooled liquid region (SLR), ranging from 80 to 130 K. The high value of reduced glass transition temperature and wide SLR agree with their good glass formation ability.
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Resumen: El presente trabajo analiza la antroponimia de la aristocracia leonesa en los siglos X y XI, a fi n de contribuir a la comprensión de las estructuras de parentesco de los grupos aristocráticos, las manifestaciones de la memoria familiar y el papel del parentesco en la construcción del poder y el prestigio social. Se plantea que la aristocracia desarrolló una antroponimia específi ca basada en la reiteración de determinados nombres propios a lo largo de las generaciones, que constituyó un importante elemento de identifi cación de la parentela y que expresó en el plano simbólico la organización de los grupos de parentesco en función de la transmisión del poder y la afi rmación del prestigio familiar.
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用X光摄影技术研究了导爆索在泥面爆炸时爆坑的发展过程,得到的各瞬时爆坑轮廓线可用椭圆方程描述,瞬时最大爆坑深度约为70~80倍药芯半径,瞬时最大爆坑宽度约为200倍药芯半径,爆坑深度随时间成对数关系增长,未见临空面对其有明显影响,临空面对爆坑的影响出现在爆坑宽度为60~80倍药芯半径之后,爆坑有回缩现象。
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介绍脉冲X光机和医用X光机的特性,应用这两种设备进行一系列饱和砂土的冲击加载实验。利用医用X光机拍摄到了饱和砂土在冲击载荷作用下产生的横断裂缝、纵向排水通道以及密实沉降的照片,得到了横断裂缝和纵向排水通道的出现规律,从而为研究饱和砂土冲击液化后结构破坏与密实沉降的机理提供了一种实验观测手段。