多次透射反射红外光谱法灵敏和准确地测量单晶硅中间隙氧和代位碳的含量

建立了室温下使用多次透射反射红外光谱法(MTR-IR)测量单晶硅中间隙氧和代位碳含量的新红外光谱吸收方法,在理论和实验上证明了MTR-IR优于常规使用的单次垂直透射红外(IR)吸收测量方法。与IR法相比较,MTR-IR法的优点为:(1)间隙氧在1107 cm^-1处和代位碳在605 cm^-1处的吸收峰与MTR-IR法中红外光透过硅片的的次数N(6~12)成线性增加的正比例关系,因此单晶硅中间隙氧和代位碳含量的检测限至少比IR法低一个数量级;(2)MTR-IR法测量薄硅片如0.2 mm的厚度时产生的干涉条纹强度是单次垂直透射红外吸收法(IR)的1/23、是单次Brewster角透射红外吸收法的1/11;(3)单次垂直透射红外吸收法(IR)1次只测量样品上的1个点,MTR-IR法则在更长的样品上1次测量多个样品点,每次测量更具有代表性。理论计算和实验结果都证实了MTR-IR吸收法测量晶体硅中间隙氧和代位碳杂质含量的高灵敏度、可靠性和重复性。     

多次透射反射红外光谱法灵敏和准确地测量单晶硅中间隙氧和代位碳的含量（英文）

建立了室温下使用多次透射反射红外光谱法(MTR-IR)测量单晶硅中间隙氧和代位碳含量的新红外光谱吸收方法,在理论和实验上证明了MTR-IR优于常规使用的单次垂直透射红外(IR)吸收测量方法。与IR法相比较,MTR-IR法的优点为:(1)间隙氧在1 107 cm-1处和代位碳在605 cm-1处的吸收峰与MTR-IR法中红外光透过硅片的的次数N(6~12)成线性增加的正比例关系,因此单晶硅中间隙氧和代位碳含量的检测限至少比IR法低一个数量级;(2)MTR-IR法测量薄硅片如0.2 mm的厚度时产生的干涉条纹强度是单次垂直透射红外吸收法(IR)的1/23、是单次Brewster角透射红外吸收法的1/11;(3)单次垂直透射红外吸收法(IR)1次只测量样品上的1个点,MTR-IR法则在更长的样品上1次测量多个样品点,每次测量更具有代表性。理论计算和实验结果都证实了MTR-IR吸收法测量晶体硅中间隙氧和代位碳杂质含量的高灵敏度、可靠性和重复性。     

超细钴纳米粒子催化1-己烯低压氢甲酰化反应的原位红外光谱研究

利用原位透射红外光谱研究了2.8 nm超细钴纳米粒子在2~3 MPa合成气(CO:H₂ = 1:1)和100 ^oC条件下催化的1-己烯氢甲酰化反应. 结果表明, 在反应中出现与Co₂(CO)₈类似的红外吸收峰(2071, 2041和2022 cm^-1), 被证明是不同Co位点端式吸附CO. 首次观测到了位于2054 cm^-1处吸收峰处的物种, 可能归属为RCH₂CH₂COCo. 通过此中间物种,产物醛可以在钴催化剂表面经由结合一个氢原子脱除反应而获得.     

用XPS和XAES分析电化学沉积的DLC膜

采用电化学沉积方法，以甲醇溶剂作碳源，直流电压作用下在单晶硅表面沉积得到碳薄膜。通过研究石墨、金刚石和样品薄膜的XPS和XAES谱图特征，证明了此方法沉积得到的是DLC薄膜;利用曲线拟合技术在C_1s电子能谱图中拟合出sp³峰与sp²峰，并计算出样品薄膜中sp³碳的相对含量为55%;研究石墨、金刚石和样品薄膜的一阶微分XAES谱图，用线性插入法估算出样品薄膜中sp³碳的相对含量为60%。     

氮化钨-钨/掺氮有序介孔碳复合材料的制备及其氧还原性能

采用软模板法制备了氮化钨-钨/掺氮有序介孔碳复合材料（WN-W/NOMC）,作为一种高比表面积且价格低廉的阴极氧还原反应催化剂。通过适量添加尿素来改变复合材料中的氮含量,在掺氮量为7%（w/w）时,实验发现材料能够保持完整有序介孔结构,测试其比表面积高达835 m²·g^-1,透射电子显微镜（TEM）测试结果显示其催化颗粒均匀地分散在氮掺杂有序介孔碳载体上。在O₂饱和的0.1 mol·L^-1 KOH溶液中测试了材料的氧还原催化性能（ORR）,显示其起始电位为0.87 V（vs RHE）,极限电流密度为4.49 mA·cm^-2,氧还原反应的转移电子数为3.4,接近于20%（w/w）商业Pt/C的3.8,说明该材料表现出近似4电子的氧还原反应途径。研究结果表明,WN-W/NOMC的催化性能虽然稍弱于商业铂碳（0.99 V,5.1 mA·cm^-2）,但其具有远超铂碳的循环稳定性和耐甲醇毒化能力。     

［La(CH2ClCOO)2(NO3)(phen)(H2O)］n的合成和晶体结构

合成了混合阴离子配合物［La(CH₂ClCOO)₂(NO₃)(phen)(H₂O)］_n。配合物经元素分析、IR、DTA-TG和UV等表征。用X射线单晶结构分析解析了标题配合物的晶体结构，三斜，空间群P1，晶胞参数为a=10.533(2)?，b=13.136(3)?，c=7.776(1)?，α=96.59(1)°，β=95.76(1)°，γ=108.42(2)°，V=1003.3(3)?³，Z=2,Dc=1.940 g/cm³, F(000)=572, μ(Mo Kα)=24.36 cm^-1。     

μ-氧-双(三苄基锡)的合成及晶体结构

用X-射线衍射方法测定了μ-氧-双(三苄基锡)的晶体结构，该化合物晶体属三方晶系，空间群为R3，晶体学参数：a=b=c=0.9646 nm，α=β=γ=83.99(1)°，V=0.8840 nm³, Z=1, D_x=1.503 g·cm^-3, μ=14.473 cm^-1, F(000)=402, R相似文献   

酚氧桥联多核铜(Ⅱ)配合物的合成、结构和磁性

利用柔性酚胺类配体N,N'-二甲基-N,N'-(2-羟基-4,5-二甲基苄基)乙二胺(H₂L)与Cu(Ⅱ)反应,合成了2个新的酚氧桥联多核Cu(Ⅱ)配合物[Cu₃^II(L)₂(CH₃OH)₂](ClO₄)₂(1),[Cu₃^II(L)₂(Cu^ICl₂)₂](2)。配合物1~2中,3个Cu²⁺之间通过2个酚氧桥连接,形成线性三核结构。两边的铜离子分别被配体L^2-上的N₂O₂螯合配位,轴向与甲醇分子的氧(配合物1)或[CuCl₂]^-的氯(配合物2)配位,形成四方锥配位构型。中间铜离子与两侧L^2-上的4个酚氧原子以平面四边形配位。Cu^II-O-Cu^II键角为100.14°~101.79°。对配合物1~2进行变温磁化率测量表明,铜离子之间通过酚氧桥存在强的反铁磁耦合,磁耦合常数J分别为-277(9)cm^-1(配合物1)和-299(3)cm^-1(配合物2)(基于自旋哈密顿算符Ĥ=-2J(Ŝ₁·Ŝ₂+Ŝ₂·Ŝ₃)。J值与酚氧桥桥联键角有一定相关性,即Cu-O-Cu桥联键角越大,反铁磁耦合越强。     

氮掺杂有序介孔碳-Ni纳米复合材料的制备及电化学性能

以F₁₂₇为模板剂,NiCl₂为镍源,尿素为氮源,间苯二酚甲醛原位聚合树脂为碳源,分别采用均相法和两相法制备Ni-N-OMC-1,Ni-N-OMC-2纳米复合材料.X射线衍射(XRD)、激光拉曼以及透射电子显微镜(TEM)等测试结果表明,复合材料具有有序介孔结构,Ni以金属微粒形式嵌于碳骨架中,提高了有序介孔碳的石墨化程度.X射线光电子能谱测试(XPS)表明尿素热解后以4种形式存在:sp³杂化与C结合的N原子,吡啶N原子,sp²杂化与C结合的N原子以及quaternary-N原子.Ni-N的共改性改变了碳载体的理化性质,有利于Pt纳米粒子的负载与分散.均相法制备的Ni-N-OMC-1复合材料微波负载Pt后,氧还原极限电流密度为5.32mA·cm^-2,氢氧化电化学活性面积高达138.53m²·g^-1,电化学催化活性优于商业20%Pt/C材料(4.49mA·cm^-2,96.98m²·g^-1).     

一维链状μ-氯(氧)-三苄基锡的合成和结构研究

合成了两种具有新型结构的苄基锡化合物：一维链状μ-氯-三苄基锡(1)和一维链状μ-氧-三苄基锡(2)，经X-射线方法测定了化合物的晶体结构。晶体结构(1)属正交晶系，空间群为P2₁2₁2₁，晶体学参数：a=0.855 3(3) nm，b=1.081 4(4) nm，c=1.968 1(7) nm，V=1.820 4(11) nm³，Z=4，D_c=1.560 g·cm^-3，μ(Mo Kα)=15.47 cm^-1，F(000)=856，R₁=0.059 7，wR₂=0.141 5。晶体结构(2)属正交晶 系，空间群为P2₁2₁2₁，晶体学参数：a=1.982 3(4) nm，b=1.089 1(2) nm，c=0.861 1(17) nm，V=1.859 0(6) nm³，Z=4，D_c=1.458 g·cm^-3， μ(Mo Kα)=13.76 cm^-1，F(000)=820，R₁=0.032 7，wR₂=0.064 8。配合物中锡原子均呈五配位畸变三角双锥构型。     

Temperature‐dependent polymorphic crystalline structure and melting behavior of poly(butylene adipate) investigated by time‐resolved FTIR spectroscopy

The polymorphic crystalline structure and melting behavior of biodegradable poly(butylene adipate) (PBA) samples melt‐crystallized at different crystallization temperatures were studied by differential scanning calorimetry (DSC) and fourier transform infrared (FTIR) spectroscopy. The crystalline structure and melting behavior of PBA were found to be greatly dependent on the crystallization temperature. By comparison of the FTIR spectra and the corresponding second derivatives between the α‐ and β‐crystal of PBA, the spectral differences were identified for the IR bands appeared at 1485, 1271, 1183, and 930 cm^?1 and the possible reasons were presented. Especially, the 930 cm^?1 band was found to be a characteristic band for the β‐crystal. Combining the DSC data with the analysis of normalized intensity changes of several main IR bands during the melting process, the melting behaviors of the α‐ and β‐crystal were clarified in detail. It is demonstrated by the in situ IR measurement that the β‐crystalline phase would transform into the α‐crystalline phase during the melting process, and the solid–solid phase transition from the β‐ to α‐crystal was well elucidated by comparing the intensity changes of the 1170 and 930 cm^?1 bands. The dependence of the β‐ to α‐crystal phase transition on the heating rate was revealed by monitoring the intensity ratio of the 909 and 930 cm^?1 band. It was suggested that at the heating rate of 0.5 or 1 °C/min, the percent amount of the transformed α‐crystal from the β‐crystal was much higher than that at the higher heating rate. The β‐crystal transforms into the α‐crystal incompletely at the higher heating rate because of the less time available for the phase transition. In addition, the β‐ to α‐crystal phase transition was further confirmed by the IR band shifts during the melting process. © 2009 Wiley Periodicals, Inc. J Polym Sci Part B: Polym Phys 47: 1997–2007, 2009     

Atomistic Simulations of CO Vibrations in Ices Relevant to Astrochemistry

The experimental absorption band of carbon monoxide (CO) in mixed ices has been extensively studied in the past. The astrophysical interest in this band is related to its characteristic shape, which appears to depend on the surrounding ice structure. Herein, molecular dynamics simulations are carried out to analyze the relationship between the structure of the ice and the infrared (IR) spectrum of embedded CO molecules at different concentrations. Instead of conventional force fields, anharmonic potentials are used for the bonded interactions. The electrostatic interactions are more accurately described by means of fluctuating atomic multipole moments (up to quadrupole). The experimentally observed splitting of the CO absorption band (gas phase: 2143 cm^?1) into a blue‐ (2152 cm^?1) and a red‐shifted (2138 cm^?1) signal is also found in the simulations. Complementary atomistic simulations allow us to relate the spectra with the structural features. The distinction between interstitial and substitutional CO molecules as the origin of this splitting is found to be qualitatively correct. However, at increasing CO concentrations, additional effects—such as mutual interactions between CO molecules—become important, and the simplistic picture needs to be revised.     

Determination of oxygen and carbon impurities in polycrystalline silicon by IR spectrometry

The possibility of using infrared spectrometry for the determination of the total oxygen and carbon impurity in polycrystalline silicon of the natural isotope composition and that enriched with the ²⁸Si isotope was studied for samples synthesized by different methods. The results of determining these impurities by the optical method are compared to those obtained by independent methods of analysis. The conditions of IR spectrometric analysis of the silicon synthesized by deposition from the gas phase are determined. It is shown that, for IR spectrometry, the upper boundaries of the analytical range of oxygen and carbon in polycrystalline silicon are 1 × 10¹⁸ and 2 × 10¹⁸ cm^?3; and the limits of their detection are 8 × 10¹⁵ and 5 × 10¹⁵ cm^?3 at a sample thickness of 0.5 and 0.2 cm, respectively.     

Photoluminescence study of silicon solar cells irradiated with large fluence electrons or protons

In order to investigate the anomalous degradation of space silicon solar cells which was found in large fluence region, photoluminescence measurements are carried out for the cells irradiated with 1 MeV electrons with a fluence exceeding 1×10¹⁶ e/cm² and 10 MeV protons with a fluence exceeding 1×10¹³ p/cm². For both irradiation, the intensity of boron-related bound exiton line decreases with fluence and it disappears at the fluences where the anomalous degradation occurs. The dominant defect is a complex of an interstitial carbon and an interstitial oxygen (C_I–O_I). The generation of five-vacancy-defects was also observed for the proton irradiation. Variations of photoluminescence line intensity are discussed in terms of displacement damage dose calculated based on non-ionizing energy loss (NIEL).     

Substitutional carbon defects in silicon: A quantum mechanical characterization through the infrared and Raman spectra

The infrared (IR) and Raman spectra of eight substitutional carbon defects in silicon are computed at the quantum mechanical level by using a periodic supercell approach based on hybrid functionals, an all electron Gaussian type basis set and the CRYSTAL code. The single substitutional C _s case and its combination with a vacancy (C _sV and C _sSiV) are considered first. The progressive saturation of the four bonds of a Si atom with C is then examined. The last set of defects consists of a chain of adjacent carbon atoms C, with i = 1–3. The simple substitutional case, C _s, is the common first member of the three sets. All these defects show important, very characteristic features in their IR spectrum. One or two C related peaks dominate the spectra: at 596 cm⁻¹ for C _s (and C _sSiV, the second neighbor vacancy is not shifting the C _s peak), at 705 and 716 cm⁻¹ for C _sV, at 537 cm⁻¹ for C and C (with additional peaks at 522, 655 and 689 for the latter only), at 607 and 624 cm⁻¹, 601 and 643 cm⁻¹, and 629 cm⁻¹ for SiC, SiC, and SiC, respectively. Comparison with experiment allows to attribute many observed peaks to one of the C substitutional defects. Observed peaks above 720 cm⁻¹ must be attributed to interstitial C or more complicated defects.     

Gas and vapor transport properties of amorphous perfluorinated copolymer membranes based on 2,2-bistrifluoromethyl-4,5-difluoro-1,3-dioxole/tetrafluoroethylene

Teflon AF 2400 (Du Pont) is an amorphous, glassy perfluorinated copolymer containing 87 mol% 2,2-bistrifluoromethyl-4,5-difluoro-1,3-dioxole and 13 mol% tetrafluoroethylene. The polymer has an extremely high fractional free volume of 0.327. Permeability coefficients for helium, hydrogen, carbon dioxide, oxygen, nitrogen, methane, ethane, propane, and chlorodifluoromethane (Freon 22) were determined at temperatures from 25 to 60°C and pressures from 20 to 120 psig. Permeation properties were also determined at a feed pressure of 200 psig at 25°C with a 2 mol% n-butane/98 mol% methane mixture. Permeabilities of permanent gases in Teflon AF 2400 are among the highest of all known polymers; the oxygen permeability coefficient at 25°C is 1600 × 10⁻¹⁰ cm³ (STP) cm/cm² s cmHg and the nitrogen permeability coefficient is 780 × 10⁻¹⁰ cm³ (STP) cm/cm² s cmHg. The permeabilities of organic vapors increase up to 20-fold as the vapor activity increases from 0.1 to unity, indicating that Teflon AF 2400 is easily plasticized. Although Teflon AF 2400 is an ultrahigh-free-volume polymer like poly(1-trimethylsilyl-1-propyne) [PTMSP], their gas permeation properties differ significantly. Teflon AF 2400 shows gas transport behavior similar to that of conventional, low-free-volume glassy polymers. PTMSP, on the other hand, acts more like a nanoporous carbon than a conventional glassy polymer.     

Bonding mechanisms and conformation of poly(ethylene oxide)-based surfactants in interlayer of smectite

A better understanding of the interactions between poly(ethylene oxide) (PEO)-based nonionic surfactants and smectite is important to fully comprehend the transport and the fate of nonionic surfactants in the environment and to design novel organo-clay composites. We studied the bonding between the surfactants and smectite and the molecular conformations of the surfactants in the interlayer of smectite. A reference polymer PEG and three nonionic surfactants—Brij 56, Brij 700, and PE-PEG—were intercalated into a smectite. The polymers and the composites were characterized with X-ray diffraction (XRD) and Fourier transform infrared (FT-IR) spectroscopy. The XRD and FT-IR results indicate that the bulk surfactants existed as crystalline materials at room temperature, and surfactant molecules had both helical/extended diblock and planar zigzag conformations. The surfactants intercalated smectite and expanded the d(001) spacing of smectite to nearly 1.8 nm. The shapes and positions of the IR bands of interlayer surfactants were similar to those of the melted (amorphous) bulk polymers: the wagging vibrations of the CH₂ merged to a single band at 1,350 cm⁻¹, the twisting bands of CH₂ had 9 cm⁻¹ or more blue shifts. These changes imply that the PEO segments of the surfactants existed with a distorted and extended conformation in the interlayer of smectite, and this extended conformation was an intermediate form of the helical and planar zigzag conformations. The molecular conformation of the interlayer surfactant was not affected by the seven types of exchangeable cations (Na⁺, K⁺, Ca²⁺, Mg²⁺, Cu²⁺, Ni²⁺, and H⁺) tested. There were 20 cm⁻¹ or more red shifts from the C–O–C stretching bands when the surfactants were adsorbed. The red shifts suggest that surfactants were bonded to smectite mainly through (1) H-bonding between oxygen atoms of the PEO segments and water molecules in hydration shells of the exchangeable cations, and (2) direct coordination or ion–dipole interaction between the oxygen atoms of the PEO segments and the exchangeable cations. With the extended conformation, the oxygen atoms of the PEO segments have maximum exposure to the bonding water molecules and exchangeable cations.     

A Global Model of Chemical Vapor Deposition of Silicon Dioxide by Direct-Current Corona Discharges in Dry Air Containing Octamethylcyclotetrasiloxane Vapor

A model of the electron distribution in direct current corona plasmas is combined with a global chemistry model and a two-dimensional transport model to predict the rate of chemical vapor deposition of silicon dioxide on the discharge wire in both positive and negative discharges in dry air containing octamethylcyclotetrasiloxane. The gas-phase chemistry includes reactions to form atomic oxygen (O) and additional global reactions to form gaseous silicon dioxide precursors by the impact reactions of electrons and atomic oxygen with silicone molecules. Surface chemistry is approximated by a single step global reaction from gaseous to solid silicon dioxide. The rate coefficient between atomic oxygen and octamethylcyclotetrasiloxane is estimated from prior experiments to be on the order of 10^–12 cm³/molecule-s. The effects of discharge polarity, current, wire radius and air velocity (Peclet number for mass transfer) on the deposition rate are considered. Deposition rates can be minimized by using positive coronas instead of negative coronas for Peclet number less than 18.5. At higher Peclet numbers, the deposition rate is slightly higher in positive corona discharges, but devices used indoors should continue to use the positive corona in order to minimize the production of ozone. The deposition rate in the positive corona is relatively insensitive to air velocity for velocities from 0.044 to 10 m/s^–1 . However,it may be minimized by operating the corona with the lowest current that provides adequate performance (e.g., particle charging) and the smallest wire that provides adequate mechanical strength.     

Au掺杂硅纳米线的稳定性和电子结构

采用基于密度泛函理论的第一性原理的方法, 对Au掺杂[100]方向氢钝化硅纳米线(SiNWs)不同位置的形成能、能带结构、态密度及磁性进行了计算, 考虑了Au占据硅纳米线的替代、四面体间隙和六角形间隙的不同位置. 结果表明: Au偏爱硅纳米线中心的替代位置. Au掺杂后的硅纳米线引入了杂质能级, 禁带宽度变窄. 对于Au替代掺杂, 杂质能级主要来源于Au的d、p态和Si的p态, 由于Au的d态和Si的p态的耦合, Au掺杂硅纳米线具有铁磁性. 对于间隙掺杂, 杂质能级主要来源于Au的s态, 是非磁性的. 另外, 根据原子轨道和电子填充模型分析了其电子结构和磁性.