高一上学期综合自测题

选择题本大题共12小题,每小题5分,共60分．在每小题给出的四个选项中,有且仅有一项是符合题目要求的。     

Hawking Radiation of a d-Dimensional Black Hole with Quantum Correction

We study the absorption probability and Hawking radiation of the scalar field in a d-dimensional black hole with quantum correction arising from the polymer quantization. We find that the quantum length scale k (i.e., the bounce radius) modifies the standard results in greybody factors and Hawking radiation on the brane and into the bulk. For the black hole with the larger mass M the effects of the parameter k in the four-dimensional black hole spacetime are entirely different from those in the high dimensional cases. When the mass of black hole M becomes very small, we also find that only the sign of the change rate of the greybody factors on the brane with respect to the dimensional number depends sharply on the bounce radius k. These information can help us know more about the extra dimension and the black holes with quantum correction.     

基于微型光谱仪的多参数水质检测微系统设计与实验

针对水资源环境监测与保护的需求,提出了基于微型光谱仪连续光谱分析的多参数水质检测微系统,系统主要由MOEMS微型光谱仪、流路系统、多功能微小型样品反应检测室和嵌入式测控系统组成,具有自动进样和试剂、样品反应体系的自动恒温、搅拌、光谱检测和数据处理等功能。论文介绍了系统各主要部分的功能与结构,研制出了原理样机,经实验测试验证,研制的多参数水质检测仪能够快速实现多个水质参数的准确检测,满足水质多参数在线监测的应用技术要求,同时具有很大的功能扩展性。     

培养学生思维的批判性例说

培养学生思维的批判性例说陈松柏（湖北省潜江中学４３３１００）培养学生的逻辑思维能力的核心是培养其思维的智力品质，而思维的智力品质的核心是思维的批判性，因而我们所求思维能力的培养，从其根本上讲就应当是培养学生的思维批判性．思维批判性的思维表象是：类比─...     

Reissner-Nordstr?m de Sitte 黑洞的引力似正模

利用P?shl-Teller势近似方法,本文研究了径向和角向引力扰动引起的Reissner-Nordstr?m de Sitte 黑洞的似正模。研究表明,当宇宙常数增加时似正模虚部的强度变小,但它却随电荷、谐波数或轨道角动量增加而增加。当电荷固定而宇宙常数改变时,似正模的虚部与实部几乎成线性关系。研究还发现径向和角向引力扰动引起的似正模是一致的,这证实似正模只依赖于黑洞的参量而与初始扰动无关。     

高二上学期综合自测题

选择题本大题共12小题,每小题5分,共60分．在每小题给出的四个选项中,有且仅有一项是符合题目要求的．     

Asymptotic Quasinormal Modes of the Garfinkle-Horowitz-Strominger Dilaton Black Hole

Using the monodromy technique proposed by Motl and Neitzke (.Adv. Theor. Math. Phys. 7(2003)307), we investigate the analytic forms of the asymptotic quasinormal frequencies for the massless scalar perturbation in the Garfinkle-Horowitz-Strominger dilaton spacetime. We find that the real parts of the quasinormal frequencies are TH ln 3. This agrees with that of the quasinormal modes in the Schwarzschild spacetime. Our result implies that Hod‘s conjecture about In 3 is still valid for the black hole spacetime in the string theory.     

Quasinormal Modes of a Coupled Scalar Field in the Acoustic Black Hole Spacetime

By using the third-order Wentzel-Kramers-Brillouin approximation and the monodromy methods, the quasnormal modes of a coupled scalar field in the canonical non-rotating acoustic black hole spacetime are investigated. It is shown that the coupling between the scalar field and background metric affects the quasinormal frequencies. At low overtones, both the real part and the magnitude of imaginary part increase with the couple factor ξ. For the larger ξ, both of them are almost linearly related to the couple factor. At high overtones, it is found that the frequency formula of the quasinormal modes is 2πω/κ = ln （ 1 ＋ 2 cos√9-24ξ/5 π） - i（2n ＋ 1）π, which means that 5 when ξ is larger, the real part is the linear function of ξ^1/2.     

Repulsive Effect for Unbound High Energy Particles Along Rotation Axis in Kerr-Taub-NUT Spacetime

We have investigated the acceleration of the unbound high energy particles moving along the rotation axis in the Kerr-Taub-NUT spacetime, and then study the dependence of the repulsive effects on the NUT charge for the particles in the spacetime. Whether the repulsive effects with the NUT charge become stronger depends on the Carter constant, the position and velocity of the particles themselves. We also present numerically the changes of the observable velocity and acceleration with the NUT charge for the unbound particles in the Kerr-Taub-NUT spacetime.     

Holographic superconductor models in the non-minimal derivative coupling theory

We study a general class of holographic superconductor models via the Stu¨ckelberg mechanism in the non-minimal derivative coupling theory in which the charged scalar field is kinetically coupling to Einstein’s tensor. We explore the effects of the coupling parameter on the critical temperature, the order of phase transitions and the critical expo- nents near the second-order phase transition point. Moreover, we compute the electrical conductivity using the probe approximation and check the ratios ω g /T c for the different coupling parameters.