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991.
孙志刚  庞雨雨  胡靖华  何雄  李月仇 《物理学报》2016,65(9):97301-097301
采用溶胶凝胶法以及静电纺丝法, 利用热处理工艺, 成功制备出了多晶锐钛矿型TiO2纳米线, 通过两线法在室温下测试单根TiO2纳米线的V-I曲线来研究其电输运性能及磁阻效应. 结果表明: 在无光照环境下其V-I曲线为不过零点的直线, 零场电阻较大, 在磁场作用下电阻下降, 表现出负磁阻效应; 紫外光辐照环境下TiO2纳米线载流子浓度增加使得电阻变小, 然而在磁场作用下电阻增大, 表现为正磁阻效应. 紫外光辐照导致的载流子浓度变化, 使得负磁阻转变为正磁阻, 我们将磁阻变化归结为d电子局域导致的负磁阻与能带劈裂导致的正磁阻两种机理相互竞争的结果.  相似文献   
992.
WeiPing Liu  ZhiHong Li  JiangJun He  XiaoDong Tang  Gang Lian  Zhu An  JianJun Chang  Han Chen  QingHao Chen  XiongJun Chen  ZhiJun Chen  BaoQun Cui  XianChao Du  ChangBo Fu  Lin Gan  Bing Guo  GuoZhu He  Alexander Heger  SuQing Hou  HanXiong Huang  Ning Huang  BaoLu Jia  LiYang Jiang  Shigeru Kubono  JianMin Li  KuoAng Li  Tao Li  YunJu Li  Maria Lugaro  XiaoBing Luo  HongYi Ma  ShaoBo Ma  DongMing Mei  YongZhong Qian  JiuChang Qin  Jie Ren  YangPing Shen  Jun Su  LiangTing Sun  WanPeng Tan  Isao Tanihata  Shuo Wang  Peng Wang  YouBao Wang  Qi Wu  ShiWei Xu  ShengQuan Yan  LiTao Yang  Yao Yang  XiangQing Yu  Qian Yue  Sheng Zeng  HuanYu Zhang  Hui Zhang  LiYong Zhang  NingTao Zhang  QiWei Zhang  Tao Zhang  XiaoPeng Zhang  XueZhen Zhang  ZiMing Zhang  Wei Zhao  Zuo Zhao  Chao Zhou  JUNA Collaboration 《中国科学:物理学 力学 天文学(英文版)》2016,59(4):642001
Jinping Underground laboratory for Nuclear Astrophysics(JUNA) will take the advantage of the ultra-low background of CJPL lab and high current accelerator based on an ECR source and a highly sensitive detector to directly study for the first time a number of crucial reactions occurring at their relevant stellar energies during the evolution of hydrostatic stars. In its first phase, JUNA aims at the direct measurements of~(25)Mg(p,γ)~(26)Al,~(19)F(p,α)~(16)O,~(13)C(α,n)~(16)O and ~(12)C(α,γ)~(16)O reactions. The experimental setup,which includes an accelerator system with high stability and high intensity, a detector system, and a shielding material with low background, will be established during the above research. The current progress of JUNA will be given.  相似文献   
993.
In 2014, the National Natural Science Foundation of China(NSFC) approved the Jinping Underground Nuclear Astrophysics laboratory(JUNA) project, which aims at direct cross-section measurements of four key stellar nuclear reactions right down to the Gamow windows. In order to solve the observed fluorine overabundances in Asymptotic Giant Branch(AGB) stars, measuring the key ~(19)F( p,α)~(16)O reaction at effective burning energies(i.e., at Gamow window) is established as one of the scientific research sub-projects. The present paper describes this sub-project in details, including motivation, status, experimental setup, yield and background estimation, aboveground test, as well as other relevant reactions.  相似文献   
994.
Ke M  He Z  Peng S  Liu Z  Shi J  Wen W  Sheng P 《Physical review letters》2007,99(4):044301
We show that by placing a metal plate next to a two-dimensional phononic crystal, acoustic waves can tunnel through the combined structure at a specific frequency that lies inside the band gap of the phononic crystal. The enhanced transmission is attributed to the coupling of the input waves with the acoustically resonant states created between the metal plate and the phononic crystal. Experiments are in excellent agreement with the theoretical predictions.  相似文献   
995.
The HyperCP Collaboration has observed three events for the decay Sigma+ -->p mu+mu- which may be interpreted as a new particle of mass 214.3 MeV. However, existing data from kaon and B-meson decays provide stringent constraints on the construction of models that support this interpretation. In this Letter we show that the "HyperCP particle" can be identified with the light pseudoscalar Higgs boson in the next-to-minimal supersymmetric standard model, the A10. In this model there are regions of parameter space where the A10 can satisfy all the existing constraints from kaon and B-meson decays and mediate Sigma+ -->p mu+mu- at a level consistent with the HyperCP observation.  相似文献   
996.
Jiang H  Wen H  Zheng X  Liu Z  Wang K  Zhang H  Guo Y 《Optics letters》2007,32(17):2580-2582
By employing the self-modulation birefringence difference in a semiconductor optical amplifier (SOA), an improved method is proposed to generate a complete optical single-sideband (OSSB) signal. Over 30 dB sideband suppression ratios (SSRs) of lower OSSB signals are obtained over a 12 dB input power range and a 36 nm wavelength span, with a maximum of over 35 dB. Upper OSSB signals with an SSR of over 15 dB are observed using a SOA for what is believed to be the first time. This method is effective even for the carrier-suppressed signal. The theory for OSSB generation in an SOA is extended and verified by experiment.  相似文献   
997.
Some photonic crystals (PCs) consisting of complex lattices of dielectric cylinders can have an effective refraction index (neffneff) of −1. Subwavelength imaging by a slab of a honeycomb PC of dielectric cylinders with neff=−1neff=1 is investigated and an open resonator with a quality factor higher than 3000 is designed with the same PC. Air–PC interfaces with low reflection are also used for the slab lens and open resonator.  相似文献   
998.
Based on the Orlov and Shulman’s M operator, the additional symmetries and the string equation of the CKP hierarchy are established, and then the higher order constraints on L l are obtained. In addition, the generating function and some properties are also given. In particular, the additional symmetry flows form a new infinite dimensional algebra , which is a subalgebra of W 1+∞.   相似文献   
999.
We have performed first-principles calculations using full-potential augmented-plane-wave method to investigate the fundamental properties of the Cd1–xZnxTe alloys. The composition dependence of the lattice constant and the bulk modulus have been estimated from total energy calculations. By means of the analytical fitting the band structures in the vicinity of the Brillouin center a complete set of effective electron- and hole-masses have also been derived. In order to further understand the effects of the chemical bonding on the above macroscopic properties we then studied the relaxation behaviors and the changes of the electronic states upon alloying for x=0.25 system. The results presented here yield a general understanding of the fundamental properties for the Cd1–xZnxTe crystals studies.  相似文献   
1000.
"利用由无乳化剂的乳液聚合法和水浮法联用技术合成得到的有序排列的聚甲基丙烯酸甲酯(PMMA)微球为硬模板,以硝酸镁为镁源,并采用硝酸镁-柠檬酸-乙醇混合溶液浸渍PMMA微球后经干燥以及先后在300 ℃恒温灼烧3 h和500 ℃恒温灼烧5 h,制备出具有有序纳米孔道结构的MgO粒子.应用X射线衍射、高分辨扫描电子显微镜、透射电子显微镜/选区电子衍射以及N2吸附-脱附法等技术表征了PMMA和MgO样品的物理化学性质.结果表明,所得PMMA微球颗粒较为均匀,粒径约为284 nm,且排列规整有序.由PMMA硬模板  相似文献   
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