Rashba自旋-轨道相互作用对一维谐振子势场中电子性质的影响

分析了Rashba自旋-轨道相互作用对一维谐振子势场中电子性质的影响,发现该自旋-轨道相互作用能够导致能级之间的自旋翻转,并且自旋翻转的性质明显依赖于自旋-轨道耦合系数和参考系坐标之间的关系.     

自旋弛豫时间测定对固体代谢物分子力学性质的研究

自旋弛豫时间测定是研究固体物质分子动力学性质的有效手段,已广泛应用于植物糖、氨基酸、维生素、肾上腺素以及睾丸激素等多类代谢物分子动力学性质的研究中. 近来上述方法也被用于其他代谢物分子动力学性质与其多晶型相变的关系以及对代谢物结构依赖性的研究. 该文将在介绍自旋弛豫时间及其测定方法的基础上,着重对自旋弛豫时间测定研究植物糖、氨基酸及其衍生物分子动力学性质的应用工作进行讨论.     

自旋极化对Kondo系统基态的影响

Anderson模型中的自旋极化效应是一个普遍存在的问题.本文从Anderson杂质模型出发,利用变分及对角化方法分析了自旋极化所引起的系统基态性质的改变,分别研究了自旋极化对Kondo单态以及高温超导两分量模型中Zhang-Rice单态稳定性的影响问题.     

随机外磁场对一维Blume-Capel模型动力学性质的影响

近几十年来,量子自旋系统的动力学性质引起了人们的广泛关注,随着研究的不断深入,随机自旋系统的性质受到了人们的重视. 利用递推关系式方法研究了高温极限下随机外磁场中自旋s=1的一维Blume-Capel模型的动力学性质, 通过计算自旋自关联函数和相应的谱密度,探讨了外场对系统动力学行为的影响.研究表明,在无晶格场的情况下, 当外场满足双模分布时,系统的动力学性质存在从中心峰值行为到集体模行为的交跨效应.当外场满足Gauss分布, 标准偏差较小时,系统也存在交跨效应;标准偏差足够大时,系统只表现为无序行为. 另外还研究了晶格场对系统动力学性质的影响,发现晶格场的存在减弱了系统的集体模行为.     

退火对FeMn钉扎自旋阀性质的影响

通过对退火后FeMn钉扎自旋阀磁性的研究表明,真空退火对自旋阀的性质有影响.低于200℃的退火能有效的提高钉扎场;退火温度高于200℃时,自旋阀的钉扎场要下降,其他性能也恶化;在300℃时,钉扎场降为零,giantmagnetoresistance(GMR)现象消失.俄歇电子能谱仪(AES)的结果表明,在自旋阀多层膜中存在着晶界扩散 关键词： 真空退火 自旋阀 晶界扩散     

串型耦合双量子点处于自旋阻塞区时磁输运性质的研究

使用双杂质安德森模型的哈密顿量,从理论上研究了串型耦合双量子点系统处于自旋阻塞区时的磁输运性质,并用主方程近似方法求解了哈密顿量.结果表明,自旋轨道耦合作用导致的双量子点间的自旋反转隧穿能够解除系统的自旋阻塞.同时也研究了超精细相互作用导致的在量子点内自旋反转和双量子点之间的自旋关联对系统的磁输运性质的影响,取得了一些有价值的结果,并对相关的物理问题进行了讨论.     

Cr掺杂浓度对AlN半金属性影响的第一性原理研究

本文基于密度泛函理论的第一性原理方法, 在广义梯度近似(GGA)下计算了掺杂过渡金属Cr原子后AlN晶体自旋极化的能带结构、分态密度等性质. 结果表明, 半金属能隙随着掺杂浓度的增大而减小. 文中以掺杂浓度为12.5%的Cr-AlN(2×2×1)为例, 分析了其自旋极化的能带结构、分态密度和磁矩等性质, 发现Cr-3d电子对自旋向下子带导带底的能量位置起决定作用. 随着掺杂浓度的增大, Cr原子间相互作用增强, Cr-3d能带向两边展宽, 导致自旋向下子带导带底的能量位置下降, 从而半金属能隙变窄.     

铁的自旋转变对菱镁矿热力学性质的影响

含铁菱镁矿(Mg,Fe)CO3是碳进入地球深部的主要载体之一,铁的进入会引起矿物物理性质的变化。采用第一性原理计算方法,研究了菱镁矿含铁及铁的自旋转变对菱镁矿热力学性质的影响。含铁菱镁矿的低自旋态体积比不含铁菱镁矿小;高自旋态在低温端的体积比不含铁菱镁矿略微增大,在高温端却减小;在所研究的温压范围内,低自旋态的体积始终比高自旋态的体积小。含铁菱镁矿高自旋态的热膨胀系数减小,而自旋转变会导致热膨胀系数增加。考虑高低两种自旋态共存时的热力学性质时,计算结果表明:自旋态共存时的热膨胀系数、速度在自旋共存区间内分别呈现异常增大峰和异常减小峰,并且这些异常变化峰随着温度的升高向高压方向移动。     

磁量子结构中二维自旋电子的隧穿输运

研究了零偏压和偏置电压作用下磁量子结构中自旋电子的隧穿输运性质. 结果表明电子自旋 输运的性质不仅取决于磁量子结构的构型、入射电子的能量和波矢, 而且取决于偏置电压. 在零偏压下, 由等同的磁垒磁阱构成的磁量子结构不具有自旋过滤的特点, 而由不等同的磁 垒磁阱构成的磁量子结构却具有较好的自旋过滤特点. 偏置电压极大地改变了磁量子结构中 电子的极化程度, 使得电子隧穿等同的磁垒磁阱构成的磁量子结构的输运性质也显著地依赖 于电子的自旋指向. 关键词： 磁量子结构 自旋电子 隧穿输运 自旋极化     

Cr掺杂浓度对AlN半金属性影响的第一性原理研究

本文基于密度泛函理论的第一性原理方法, 在广义梯度近似(GGA)下计算了掺杂过渡金属Cr原子后AlN晶体自旋极化的能带结构、分态密度等性质. 结果表明, 半金属能隙随着掺杂浓度的增大而减小. 文中以掺杂浓度为12.5%的Cr-AlN(2×2×1)为例, 分析了其自旋极化的能带结构、分态密度和磁矩等性质, 发现Cr-3d电子对自旋向下子带导带底的能量位置起决定作用. 随着掺杂浓度的增大, Cr原子间相互作用增强, Cr-3d能带向两边展宽, 导致自旋向下子带导带底的能量位置下降, 从而半金属能隙变窄.     

质子自旋性质的研究

考虑了正、反海夸克对和胶子混杂态对质子波函数的影响，质子的一些自旋相关性质：轴矢流耦合常数ＧＡ／ＧＶ，结构函数ｇ１ｎ和ｇ１ｐ的计算得到了改进．     

Sea quark contributions to nucleon electromagnetic form factors with the nonlocal chiral effective Lagrangian

The sea quark contributions to the nucleon electromagnetic form factors of the up,down and strange quarks are studied with the nonlocal chiral effective Lagrangian.Both octet and decuplet intermediate states are included in the one loop calculations.Compared with the strange quark form factors,although their signs are the same,the absolute value of the light quark form factors are much larger.For both the electric and magnetic form factors,the contribution of the d quark is larger than of the u quark.The current lattice simulations of the light sea quark form factors are in between our results for the u and d quarks.     

Toy model of the repulsive core of the nucleon-nucleon potential

We study the simplest quark model assuming that the sea of gluons and quark-antiquark pairs can be treated as a part of a static force and proceeding to calculate the hadronic states by solving the Schrödinger equation for a static confining interaction. We refer to this model, starting from a system of six interacting constituent quarks, and examine how the picture of two structureless nucleons can change when the effects caused by the substructure of the nucleons are taken into account.     

Determining the strange and antistrange quark distributions of the nucleon

The difference between the strange and antistrange quark distributions,δs(x) = s(x) ˉs(x),and the combination of light quark sea and strange quark sea,Δ(x) =ˉ d(x) + uˉ(x) s(x) ˉs(x),are originated from non-perturbative processes and can be calculated using non-perturbative models of the nucleon.We report calculations of δs(x) and Δ(x) using the meson cloud model.Combining our calculations of Δ(x) with relatively well known light antiquark distributions obtained from global analysis of available experimental data,we estimate the total strange sea distributions of the nucleon.     

Is There Really a Spin Crisis?

The matrix element of quark axial vector current is shown to be different from the nonrelativistic quark spin sum for a nucleon at rest. The nucleon spin content discovered in polarized deep inelastic scattering is shown to be accommodated in a constituent quark model with 15% sea quark component mixing. The relativistic correction and sea quark pair excitation inherently related to quark axial vector current reduce the nucleon axial charge and this reduction is compensated by the relativistic quark orbital angular momentum exactly and in turn keeps the nucleon spin 1/2 untouched. Nucleon tensor charge has similar but smaller relativistic and sea quark pair excitation reduction.     

Chiral Soliton with Influence on Sea Quark

The solution of the chiral soliton with influence on the sea quark is studied in the one-loop approximation. The coupled equations of the motion for the quark and the chiral field are solved numerically by the self-consistent iterative method. The exact quark density of a hedgehog baryon is compared with the results of two kinda of approximations for the chiral angle. It is found that the influence of the chiral soliton on the sea quark can not be ignored.in the calculation of the energy structure or the distribution of the quark density of a baryon.     

THE SEA QUARKS IN PAIRING VIBRATIONAL MODEL OF MESONS AND OZI RULE

A pairing vibrational model of meson with J^P=1^- is discussed including their energy spectra, configurations and decay mechanism. While the mixing configurations of valence quarks as well as the sea quark pairs in vacuum are taken into account, it is possible to propose a classification for hadronie decay of mesons and thereby a corresponding explanation of OZI rule.     

Flavor decomposition of the sea-quark helicity distributions in the nucleon from semiinclusive deep inelastic scattering

Double-spin asymmetries of semiinclusive cross sections for the production of identified pions and kaons have been measured in deep inelastic scattering of polarized positrons on a polarized deuterium target. Five helicity distributions including those for three sea quark flavors were extracted from these data together with reanalyzed previous data for identified pions from a hydrogen target. These distributions are consistent with zero for all three sea flavors. A recently predicted flavor asymmetry in the polarization of the light quark sea appears to be disfavored by the data.     

Polarized parton distribution in the relativistic quark exchange framework

The Spin dependent gluon and sea quark distributions of the proton and the neutron are extracted in the leading order (LO) and the next-to-leading order (NLO) QCD. The relativistic quark exchange model is used to calculate the related valence quark spin dependent structure function. The inverse Mellin transform technique is performed to evaluate the polarized x-dependent distributions of the gluon and the sea quark from the various moments of the valence quarks. It is shown that the calculated spin structure functions (SSF) of the proton and the neutron are in good agreement with the available data, such as E143, SMC, E142, E154 and Hermes experiments. A comparison is also made with the other theoretical models. Finally it is shown that the above calculated parton distributions improve the SSF of the proton and the neutron. Received: 4 January 1999 / Revised version: 12 April 1999