锂离子电池掺钴正极材料电子结构的DV-Xα研究

采用原子基表示的第一原理赝势方法 ,计算了正极材料LiMn2 O4的电子结构 ,发现LiMn2 O4的价带主要是由Mn(8)和Mn(9)的 3d轨道和O(7)、O(6 )、O(4 )的 2p轨道构成 ,导带主要是由Mn(8)和Mn(9)的 3d轨道和O(7)的 2 p轨道构成 .通过计算Li5Mn7CoO8的电子结构 ,发现在LiMn2 O4中用钴离子取代 16d位锰离子将使电极材料的费米能减小 ,放电电压降低 ;锂离子的净电荷增大 ,锂离子与氧离子的相互作用增强 ,可逆容量降低 ;同时由于价带宽度变窄 ,Co-O键间的相互作用比Mn -O键间的相互作用强 ,所以 ,结构稳定性增加 ,电极循环性能改善 .     

锂离子电池掺钴正极材料电子结构的DV-Xa研究

采用原子基表示的第一原理赝势方法，计算了正极材料LiMn2O4的电子结构，发现LiMn2O4的价带主要是由Mn(8)和Mn(9)的3d轨道和O(7)、O(6)、O(4)的2p轨道构成，导带主要是由Mn(8)和Mn(9)的3d轨道和O(7)的2p轨道构成．通过计算Li5Mn2C0O8的电子结构，发现在LiMn2O4中用钴离子取代16d位锰离子将使电极材料的费米能减小，放电电压降低；锂离子的净电荷增大，锂离子与氧离子的相互作用增强，可逆容量降低；同时由于价带宽度变窄，Co-O键间的相互作用比Mn-O键间的相互作用强，所以，结构稳定性增加，电极循环性能改善．     

Mn掺杂Mo2 FeB2的电子结构，磁性和弹性的第一性原理研究

用第一性原理计算（ Mo,Fe,Mn）3 B2的结构稳定性、磁性、电子结构和弹性。过程中采用了密度泛函理论和超软赝势。研究表明反铁磁性具有最低的能量,为基态。计算所得的（ Mo,Mn,Fe） B2电子态密度和布局数与Mo2 FeB2的类似。从电子态密度和重叠布局数发现,B?B和B?Mo为共价键,对剪切模量起促进作用。通过磁性分析,发现Fe和Mn原子起主要作用。然而,Mn的掺杂对硬质相Mo2 FeB2的成键和弹性的影响微小。     

Cr、Mn、Co、Ni掺杂对Al13Fe4相稳定性和力学性能影响的第一性原理研

采用基于密度泛函理论的第一性原理计算方法,系统地研究了不同掺杂浓度下过渡族元素Cr、Mn、Co、Ni在Al13Fe4相中的占位情况、结构稳定性和机械性能. 计算得到所有的Al13(Fe24-xMx) (M=Cr、Mn、Co、Ni;X=1,2,4)相都具有良好的热力学稳定性和机械稳定性. 相同掺杂浓度化合物的形成焓按如下顺序减小：Al78(Fe24-xCrx) > Al78(Fe24-xMnx) > Al13Fe4 > Al78(Fe24-xNix) > Al78(Fe24-xCox).形成焓的降低增加了Al13Fe4相成核驱动力,Co和Ni有利于促进Al-Fe合金中Al13Fe4相形核,细化Al13Fe4相. 过渡族元素可以改善金属间化合物的脆性,增强塑性变形能力. 并且随着掺杂浓度的增加,过渡族元素的加入对脆性的改善呈先增大后减小的趋势.     

Mn2+、N2-共掺杂Zn2GeO4晶体电子结构和光学性质的研究

采用基于密度泛函理论的平面波超软赝势方法对本征Zn2GeO4，Mn2+掺杂Zn2GeO4，Mn2+/N2-共掺杂Zn2GeO4超晶胞进行了几何结构优化，计算了掺杂前后体系的晶格常数、能带结构、态密度和光学性质。结果表明，Mn离子掺入后，Mn离子3d轨道与O离子2p轨道之间有强烈的轨道杂化效应，掺杂系统不稳定，而Mn/N离子共掺后，Mn离子和N离子之间的吸引作用克服了Mn离子之间的排斥作用，能够明显地提高掺杂浓度和体系的稳定性。光学性质计算结果表明，Mn离子与N离子共掺杂能改善Zn2GeO4电子在低能区的光学跃迁特性，增强电子在可见光区的光学跃迁；吸收谱计算结果显示，Mn离子与N离子掺入后体系对低频电磁波吸收增加。     

掺杂ZnTe对电子结构与磁性质的影响

为了研究Mn、Fe、Co、Ni掺杂ZnTe的电子结构和磁性的相关性质.本文基于第一性原理的数值基组的方法计算了Mn、Fe、Co、Ni掺杂ZnTe的能带结构、态密度,分析了掺杂结构的稳定性和磁性性质.结果发现Mn、Fe、Co、Ni掺杂ZnTe的杂质替换能分别为-1.14 e V,-1.23 e V,39.95 e V,-4.32 eV,表明Mn、Fe、Ni掺杂的ZnTe在实验上较容易实现.Mn、Co掺杂ZnTe导致体系产生的总磁矩分别为0.997μB,1.103μB,其中磁性的主要来源于Mn、Co原子在Zn位的取代而引起,产生局域磁性主要取决于Mn、Co的d轨道与Te的p轨道耦合作用.     

Mn掺杂6H-SiC的第一性原理研究

本文通过密度泛函理论第一性原理平面波超软赝势计算方法计算了Mn掺杂6H-SiC的电子结构与光学性质。计算结果显示掺杂Mn后的6H-SiC为间接带隙p型半导体,且带隙较本征体有所降低,带隙由2.022 eV降为0.602 eV,电子从价带跃迁所需能量减少。掺杂后的Mn的3d能级在能带结构中以杂质能级出现,提高了载流子浓度,导电性增强。光学性质研究中,掺杂Mn后的介电函数虚部在低能处增加,电子激发态数量增多,跃迁概率增大。掺杂后的光吸收谱能量初值也较未掺杂的3.1 eV扩展到0 eV,反射谱发生红移。由于禁带宽度的降低使得光电导率起始范围得到扩展。     

掺杂Fe对VH2解氢性能影响的第一性原理研究

采用密度泛函理论(DFT)的第一性原理的平面波超软赝势方法,研究了Fe掺杂对VH₂的电子结构和解氢性能的影响.通过计算Fe掺杂VH₂前后体系的合金形成热、V-H之间的重叠布居数、电子态密度、电子密度,发现Fe掺杂VH₂后,随着Fe含量增加,合金体系的晶胞参数和晶胞体积逐渐减少;体系的负合金形成热逐渐减少,且掺杂后体系的负合金形成热都比VH₂的负合金形成热小,体系的稳定性降低;电子态密度计算也显示Fe掺杂后费米能级处的电子浓度增加,体系稳定性降低;重叠布居数和电子密度计算表明掺杂后V-H之间的重叠布居数由0.1减小为0.08或0.09,V-H之间的电子密度减少,说明V和H原子之间的相互作用减弱,提高了VH₂的解氢性能.计算结果解释了实验现象. 关键词： Fe掺杂 电子结构 解氢性能 第一性原理计算     

第一性原理计算：锰酸锂掺杂Fe和Co的性质研究

文章基于密度泛函理论的第一性原理计算,研究了LiMn2O4电池材料在掺杂Fe和Co离子时的电子结构和电化学性能。发现Fe\Co取代Mn3+在热力学上是会更加稳定,提升电化学性能。掺杂Fe后,LiMn2O4电池材料晶格参数减小(约0.3%);掺杂Co后,LiMn2O4电池材料晶格参数减小(约0.5%)。这两种掺杂方式让与之相邻的Mn3+被氧化成Mn4+,从而降低了Jahn-Teller畸变情况产生可能性。对于掺Fe尖晶石型锰酸锂(Li8Mn15FeO32),Mn环境中的Li离子会更容易被提取,第一次放电电压从原来的3.7V增加至4.623V;对于掺Co尖晶石型锰酸锂(Li8Mn15CoO32),第一次放电电压从原来的3.7V增加至4.101V。研究为锂电池电容量研究提供理论数据的参考。     

AlSb掺Mn、Fe的电子结构和光学性质

采用基于密度泛函理论(DFT)的平面波超软赝势(PWPP)方法,对Mn、Fe掺杂前后AlSb的超晶胞体系进行了几何结构优化.模拟计算了Mn、Fe掺杂对AlSb的电子结构和光学性质的影响,分析了掺杂前后的能带结构、电子态密度分布、电荷布局分布、介电常数和光吸收系数的变化.计算结果表明:在Mn,Fe单掺杂AlSb体系中,由于空穴密度的增加,禁带宽度减小,材料表现出半金属行为,且在可见光区电子跃迁明显增强.     

Anharmonic properties of rocksalt structure solids

An effort has been made for obtaining the anharmonic properties of rocksalt structure solids starting from primary physical parameters viz. nearest-neighbor distance and hardness parameter assuming long- and short-range potentials at elevated temperatures. The elastic energy density for a deformed crystal can be expanded as power series of strains for obtaining coefficients of quadratic, cubic and quartic terms which are known as the second-, third- and fourth-order elastic constants, respectively. When the values of the higher-order elastic constants are known for a crystal, many of the anharmonic properties of the crystal can be treated within the limit of the continuum approximation in a quantitative manner. In this study, higher-order elastic constants are computed up to their melting temperature for rocksalt structure solids, which are alkali cyanides, sodium and potassium halides. The first order pressure derivatives of second- and third-order elastic constants, the second-order pressure derivatives of second-order elastic constants and partial contractions are also evaluated at different temperatures for these substances. The results thus obtained are compared with experimental data and found in well agreement with present values.     

Possible thermal structure of the eastern part of the Central Alps

Summary This is a survey of the trend of temperature in respect of depth in the lithosphere under the eastern part of the Central Alps between Innsbruck and Graz, using a geothermal model based on the reduced heat production along the vertical and on the thermal, conductivity dependence upon temperature and pressure. A linear relationship has been found between the reduced heat flow and the mean surface heat flow; it was thus possible to estimate the radiogenic heat flow produced by the sialic crust and the heat flow entering its base. The geotherm corresponding to the surface heat flow in combination with the melting point curves of granitic and gabbroic rocks and with the mantle solidus was used to explain the observed low-velocity zones in the crust and to determine the depth of the lithosphere-asthenosphere transition.

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Riassunto Si studia l'andamento della temperatura con la profondità nella litosfera sotto il settore orientale delle Alpi Centrali, compreso tra Innsbruck e Graz, per mezzo di un modello geotermico che tiene conto della diminuzione di produzione di calore lungo la verticale e della dipendenza della conducibilità termica dalla temperatura e dalla pressione. Si è trovata una relazione lineare tra il flusso di calore ridotto e quello medio alla super-ficie, che ha permesso di stimare il flusso di calore radiogenico prodotto dalla crosta sialica e quello entrante alla sua base. La geoterma corrispondente al flusso di calore superficiale è stata confrontata con le curve di fusione di rocce granitiche e gabbriche e con il solidus del mantello, per spiegare le zone crostali a bassa velocità e per determinare la profondità del confine litosfera-astenosfera.

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Резюме Используя геотермальную модель, основанную на уменьшении выделения тепла вдоль вертикали и на зависимости удельной теплопроводности от температуры и давления, анализируется распределение температур по глубине в литосфере под восточной частью центральных Альп между Иннсбруком и Грацем. Получено линейное соотношение между потоком приведенного тепла и средним потоком тепла с поверхности. Таким образом, можно оценить радиоактивный поток тепла из земной коры и поток тепла, входящий в основание. Геотерма, соответствующая потоку поверхностного тепла, сравнивается с кривыми плавления гранитных и вулканических пород и криавой твердой мантии, чтобы обьяснить зоны с малыми скоростями в земной коре и определить глубину границы между литосферой и астеносферой.

     

(CdSe)n(n=1,2)团簇性质及CdSe分子热力学性质的理论计算

用密度泛函B3LYP方法、有效核势(ECP)基组LanL2DZ对(CaSe)n(n=1,2)团簇进行了理论研究,得到(CaSe)n(n=1,2)分子体系可能存在的状态及各电子状态的平衡几何Re、谐振频率、偶极矩和离解能De、不同温度、压力下的热力学函数值;设用总能量中的电子和振动能量近似代表CdSe分子处于固态时的能量,用总熵中的电子和振动熵近似代表CdSe分子处于固态时的熵,进而计算了Cd与Se反应的△Hθ、△Sθ、△G,并由此计算出不同温度的反应平衡常数Kp结果表明:在298～1400K温度范围内,Cd与Se反应的自由能值均为负,且随着温度的升高,△Gθ值负的越多,表明在这个温度范围内反应能自发发生,而且自发趋势随温度的升高逐渐增大;平衡常数逐渐减小,即反应进行程度随温度的升高逐渐减小;CdSe分子材料的导电性随压力增大而增强.     

Structural,elastic and thermodynamic properties of the tetragonal structure of germanium carbonitride

The structural, mechanical, electronic and thermodynamic properties of the tetragonal structure germanium carbonitride (t-GeCN) were first investigated using the density function theory with the ultrasoft psedopotential scheme in the frame of the generalized gradient approximation and the local density approximation. The elastic constants have confirmed that the t-GeCN is mechanically stable and phonon spectra have confirmed that the t-GeCN is dynamically stable. The anisotropy studies show that t-GeCN exhibits a larger anisotropy in its Poisson's ratio, Young's modulus, shear modulus, sound velocities and universal elastic anisotropy index. Electronic structure study shows that t-GeCN is an indirect semiconductor with band gap of 0.628 eV. The thermodynamic properties of t-GeCN, including Debye temperature, heat capacity, Grüneisen parameter and thermal expansion coefficient are investigated utilizing the quasi-harmonic Debye model.     

后钙钛矿CaRhO3的电子结构和磁学性质的第一性原理研究

采用基于密度泛函理论的投影平面波方法,对后钙钛矿结构(Ppv)的CaRhO₃的电子结构和磁学性质进行了研究.广义梯度(GGA)近似下的计算表明,Ppv-CaRhO₃的基态为铁磁性半金属,Rh⁴⁺离子的磁矩大小为0.57μ_B,具有低自旋态构型;而考虑在位库仑作用修正的GGA+U计算,得到了与实验结果相符的反铁磁绝缘体基态,表明后钙钛矿结构中4d电子之间的关联效应对体 关键词： 电子结构 磁学性质 金属绝缘体转变     

贵金属氮化物晶体结构、电子结构和力学性能的实验与理论研究进展

氮化铂（Pt-N）是高温高压条件下合成的第一种块体二元贵金属氮化物，由于该化合物具有高的体弹性模量和特殊的电子结构从而吸引了世界范围内一些理论研究者的目光．Pt-N中金属原子的质量远远大于非金属原子的质量，因此X射线衍射仅能确定Pt原子的位置，拉曼光谱虽然能限制N原子的对称性，但仍不能确定其具体位置．以上因素使得确定这种新合成物质的晶体结构成了理论研究的焦点，这些工作已经在高压科学中开拓了一个新的领域，即贵金属元素氮化物的高压合成与物性研究．     

Electronic structure and magnetic properties of the compound CeCuIn

Magnetization, magnetic susceptibility, electrical resistivity, thermoelectric power and X-ray photoemission measurements were performed on a polycrystalline sample of CeCuIn. This compound crystallizes in a hexagonal structure of the ZrNiAl type. The magnetic data indicate that CeCuIn remains paramagnetic down to 1.9 K with a paramagnetic Curie temperature of −13 K and an effective magnetic moment equal to 2.5 μ_B. The electrical resistivity has metallic character, yet in the entire temperature range studied here, it is a strongly nonlinear function of temperature. The temperature dependence of the thermoelectric power is dominated by a small positive maximum near 76 K and a deep negative minimum at about 16 K. Above 150 K the thermopower exhibits a Mott's type behavior. The positive sign of the Seebeck coefficient in this temperature region indicates that the holes are dominant charge and heat carriers. The structure of Ce 3d_5/2 and Ce 3d_3/2 XPS spectra has been interpreted in terms of the Gunnarsson-Schönhammer theory. Three final-state contributions f⁰, f¹ and f² are clearly observed, which exhibit a spin-orbit splitting Δ_SO≈18.7 eV. The appearance of the 3d⁹f⁰ component is a clear evidence of the intermediate valence behavior of Ce. From the intensity ratio I(f⁰)/[I(f⁰)+I(f¹)+I(f²)] the 4f-occupation number is estimated to be 0.95. In turn, the ratio I(f²)/[I(f¹)+I(f²)]=0.08 yields a measure of the hybridization energy that is equal to 45 meV.     

Band structure,electron-phonon interaction and superconductivity of yttrium hypocarbide

Band parameters and superconductivity of yttrium hypocarbide (Y₂C) have been investigated. The computations are performed using first-principles pseudopotential method within a generalized gradient approximation. The equilibrium lattice parameters have been determined and compared with experiment. Moreover, the material of interest is found to be stiffer for strains along the a-axis than those along the c-axis. A band-structure analysis of Y₂C implied that the latter has a metallic character.The examination of Eliashberg Spectral Function indicates that Y-related phonon modes as well as C-related phonon modes are considerably involved in the progress of scattering of electrons. By integrating this function, the value of the average electron-phonon coupling parameter (λ) is found to be 0.362 suggesting thus that Y₂C is a weak coupling Bardeen-Copper-Schrieffer superconductor. The use of a reasonable value for the effective Coulomb repulsion parameter (μ* = 0.10) yielded a superconducting critical temperature T_c of 0.59 K which is comparable with a previous theoretical value of 0.33 K. Upon compression (at pressure of 10 GPa) λ and T_c are increased to be 0.366 and 0.89 K, respectively, showing thus the pressure effect on the superconductivity in Y₂C.The spin-polarization calculations showed that the difference in the total energy between the magnetic and non-magnetic Y₂C is weak.     

Electronic structure and magnetic properties of BaTi1-xMnxO3

The electronic structure and magnetic properties of polycrystalline BaTi_1-xMn_xO₃ (x = 0–0.1) compounds prepared by solid-state reactions were studied. The results revealed that the increase in Mn content (x) did not change the oxidation numbers of Ba (+2) and Ti (+4) in BaTi_1-xMn_xO₃. However, there is the change in Mn valence that Mn^3+,4+ ions coexist in the samples with x = 0.01–0.04 while Mn⁴⁺ ions are almost dominant in the samples with x = 0.06–0.1. We also point out that Mn³⁺ and Mn⁴⁺ ions substitute for Ti⁴⁺ and prefer locating in the tetragonal and hexagonal BaTiO₃ structures, respectively, in which the hexagonal phase constitutes soon as x = 0.01. Particularly, all the samples exhibit room-temperature ferromagnetism. Ferromagnetic order increases with increasing x from 0 to 0.02, but decreases as x ≥ 0.04. We think that ferromagnetism in BaTi_1-xMn_xO₃ is related to lattice defects and/or exchange interactions between Mn³⁺ and Mn⁴⁺ ions.     

Cu2Se电子结构和光学性质的第一性原理计算

采用基于密度泛函理论(DFT)的第一性原理的平面超赝势方法计算研究了Cu2Se的电子结构、态密度和光 学性质。能带结构分析表明Cu2Se为半金属、上价带主要由Se的4p电子构成下价带主要由Cu的3d电子构成静态介电常数为1.41折射率为7.74吸收系数在可见光范围内最小值为1×105cm−1且在高能区对光子的吸收减小为零其电子能量损失峰在26.84eV正好对应反射系数急剧下降的位置光电导率的波谷出现的能量范围与前面的吸收系数和消光系数的峰值和波谷出现的位置完全对应。