Probing the Microscopic Origin of Gravity via Precision Polarization and Spin Experiments

As in other parts of physics, we advocate the interaction approach: experiments ←→ (… are influenced and their importance is determined by … and vice versa) phenomenology ←→ low-energy effective (field) theory ←→ microscopic theory to probe the microscopic origin of gravity, Using the X-g phenomenological framework, we discuss the tests of equivalence principles. The only experimentally unconstrained degree of freedom is the axion freedom. It has effects on the long-range astrophysical/cosmological propagation of electromagnetic waves and can be tested/measured using the future generation of polarization measurement of cosmic background radiation.The verification or refutal of this axionic effect will be a crucial step for constructing an effective theory and probing the microscopic origin of gravity. The interaction of spin with gravity is another important clue for probing the microscopic origin of gravity. The interplay of experiments, phenomenology and effective theory are expounded. An ideal way to reveal the microscopic origin of gravity is to measure the gyrogravitational ratio of particles, Three potential experimental methods are considered.     

Deposition of Hydrogen-Free Silicon Nitride Thin Films by Microwave ECR plasma Enhanced Magnetron Sputtering at Room Temperature

Hydrogen-free silicon nitride （SiNx） films were deposited at room temperature by microwave electron cyclotron resonance （MW-ECR） plasma enhanced unbalance magnetron sputtering system. Both Fourier-transform infrared spectroscopy and x-ray photoelectron spectroscopy are used to study the bonding type and the change of bonding structures of the silicon nitride films. The results indicate that the chemical structure and composition of SiNx films deposited by this technique depend strongly on the N2 flow rates, the stoichiometric SiNx film, which has the highest hardness of 22.9 GPa, could be obtained at lower N2 flow rate of 4 sccm.     

Spin Squeezing and Entanglement of Many-Particle Spin-Half States

In many-particle spin-half systems with exchange symmetry, we find that the spin squeezing is related to two types of entanglement, the bipartite and the pairwise entanglement. A quantitative relationship is revealed for the spin squeezing parameter, the tangle, and the concurrence. We find that a class of states is spin squeezed if the pairwise entanglement is stronger than the bipartite entanglement.     

空间技术回顾与简介

 空间技术,又称航天技术,它是探索、开发利用太空及地球以外天体的一门综合技术;它包括运载工具的研制,航天器的发射、控制,以及宇航员生命保障系统的研制等。空间技术作为当代高技术门类之一,越来越受到世界各国的重视与关注。神舟飞船的3次试航成功极大地激发了国人对空间技术的兴趣,增进了对空间技术的了解。一、空间与空间技术历史的回顾探索宇宙的奥秘,奔向遥远的太空是人类自古以来追求的目标,在古希腊神话中,雅典杰出的建筑师代达罗斯,用麻线和蜜蜡将羽毛连接成翅膀插在身上,带他的孩子伊卡罗斯扇动翅膀逃出了囚禁他们的克里特岛;中国古代也有嫦娥奔月的神话传说。     

关于图的最小覆盖算法

本文就数学建模课的教学过程中 ,在“图的方法建模”一章中 ,关于图的最小覆盖法提出启发式算法 .用书中所给方法推出一个反例 ,分析了其产生错误的原因 ;通过对图的最小覆盖的概念的理解、结合分析图的关联矩阵的特点 ,给出了图的最小覆盖的启发式算法 .     

连续激光诱导Zn/InP掺杂过程中温度分布的解析计算

在实验的基础上，分析表面蒸发Zn的InP样品在连续激光诱导下掺杂Zn过程.在一维热传导问题的第三类边界条件下，给出激光辐照有限厚双层材料Zn/InP温度分布的一种直观简洁的解析形式. 关键词： 激光诱导掺杂 Zn/InP 温度分布     

EPT／BIIR橡胶密封材料制备及其性能

为了探索具备低水蒸气透过系数、低透气系数、低压缩永久变形以及良好耐老化性能的新型橡胶密封材料，鉴于影响并用胶性能的主要因素是共混相容性以及硫化速度，从实现并用胶优势互补角度出发，优选综合性能较好的三元乙丙橡胶（EPT）和溴化丁基橡胶（BIIR），开展了EPT／BIIR共混共硫化技术研究，并开展了DBPMH／HVA-2过氧化物硫化体系在EPT／BIIR并用胶中的应用研究。     

Raman properties embeddedof GaSb nanoparticlesin SiO2 films

The Raman shifts of nanocrystalline GaSb excited by an Ar^ ion laser at wavelengths 514.5, 496.5, 488.0, 476.5,and 457.9nm are studied by an SPEX-1403 laser Raman spectrometer respectively, and they are explained by phonon confinement, tensile stress, resonant Raman scattering and quantum size effects. The Stokes and anti-Stokes Raman spectra of GaSb nanocrystals strongly support the Raman feature of GaSb nanocrystals. The calculated optical spectra compare well with experimental data on Raman scattering GaSb nanocrystals.     

修正的Shepard型算子的Lp-逼近

摘要:本文在L_[0.1]~p空间给出了 Durrmeyer型修正的shepard算子D_n(f,x),对 f∈L_[0.1]~p,(p≥1),得到了下列的Jackson型估计:││D)n(f)-f││_p≤ C_(pλω)(f,n~(-1))p,λ≥2, Cω(f,n~(-1)logn)p,λ=2, C_(pλω)(f,n~(-1))p,1<λ<2,