Quantum radiation of non-stationary Kerr－Newman－de Sitter black hole

By introducing a new tortoise coordinate transformation, we investigate the quantum thermal and non-thermal radiations of a non-stationary Kerr--Newman--de Sitter black hole. The accurate location and radiate temperature of the event horizon as well as the maximum energy of the non-thermal radiation are derived. It is shown that the radiate temperature and the maximum energy are related to not only the evaporation rate, but also the shape of the event horizon, moreover the maximum energy depends on the electromagnetic potential. Finally, we use the results to reduce the non-stationary Kerr--Newman black hole, the non-stationary Kerr black hole, the stationary Kerr--Newman--de Sitter black hole, and the static Schwarzshild black hole.     

氯苯的同步辐射光电离研究

利用真空紫外同步辐射和反射式飞行时间质谱仪对氯苯进行了光电离研究,通过测量各离子的光电离效率(PIE)曲线,得到了氯苯的电离势为(9.11±0.05)eV及两种主要碎片离子C6H+5和C4H+3的出现势分别为(12.96±0.05)和(16.27±0.05)eV.结合有关文献的热力学数据,推导出C6H5Cl+、C6H+5及C4H+3的离子生成焓及一些键的解离能.实验获得了118.0nm同步辐射光电离下氯苯的质谱图.     

On the bremsstrahlung background correction to the high-energy Compton spectroscopy

methodology for bremsstrahlung (BS) background correction to extract a true Compton profile in high-energy Compton scattering experiments is presented. The BS background profiles for Hg, computed within the Born approximation, are estimated for different values of incident energy. It is seen for the first time that the BS background contribution in high-energy Compton profile experiments like those employing third generation synchrotron radiation sources comes out to be significant and non-linear. Further, it is found that the incorporation of BS correction in data reduction of such an experiment performed on Hg at 662 keV energy helps in reconciliation of theory and experiment.     

同步辐射硬x射线衍射增强成像新进展

对于相位衬度成像的实验方法研究及其在医学、材料等领域的应用研究已成为国际上研究的热点.衍射增强成像方法(DEI)作为其中的一种方法通过测量相位衬度的一阶导数而成像.在北京同步辐射装置(BSRF)4W1A束线上，对衍射增强成像方法进行了研究，并对一系列生物医学样品及材料样品成像，得到了非常清晰的相位衬度图像. 关键词： 衍射增强成像 同步辐射 硬x射线     

增强UV-B辐射、NaCl胁迫及其复合处理对小麦幼苗光合作用及黄酮代谢的影响

依据增强UV-B辐射、NaCl胁迫及其复合处理不同天数，分别测定各处理小麦幼苗第一片真叶的净光合速率、气孔导度、叶肉细胞间隙二氧化碳浓度、叶绿素含量、黄酮含量和苯丙氨酸裂解酶活性.发现NaCl胁迫和增强UV-B辐射均明显降低小麦幼苗的净光合速率、气孔导度和叶肉细胞间隙CO2浓度;和NaCl胁迫相较， NaCl+UV-B辐射对小麦幼苗上述指标无进一步降低效应.增强UV-B辐射、NaCl胁迫及其复合处理均促进苯丙氨酸裂解酶活性和黄酮含量提高.说明了增强UV-B辐射降低小麦幼苗净光合速率的主要原因是气孔限制，而NaCl胁迫减轻了增强UV-B辐射对小麦幼苗光合作用的降低效应.     

Electron-stimulated desorption of thin epitaxial films of KBr grown on (100)InSb

We have measured time-of-flight (TOF) distributions of Br atoms desorbed from thin (less than 1000 Å) epitaxial films of KBr on (100) InSb with a 2 keV electron beam. Although the general structure of the TOF spectra was similar to that obtained previously for the thick crystals, both the fast and the slow (thermal) components of the distribution were strongly dependent on the film thickness. We argue that this dependence is due to two different diffusion processes involved in the transport of the primary excitation products from the bulk to the surface. By measuring the velocity resolved ESD yield for films of various thicknesses, we determined that a diffusion length of the carriers responsible for the thermal ESD component varied from 30 to 700 Å with temperature in the range 20–300°C. In contrast, for the non-thermal desorption we found the carrier diffusion length of about 140 Å which did not depend significantly on the temperature.     

辐射驱动内爆温度源脉冲整形研究

辐射驱动温度源脉冲整形是获得高压缩比的重要途径。本文从脉冲整形的基本原理出发，采用数值模拟方法，给出适合于神光Ⅲ装置内爆实验的辐射驱动温度源脉冲整形曲线。     

Evaluating shielding effectiveness for reducing space radiation cancer risks

We discuss calculations of probability distribution functions (PDF) representing uncertainties in projecting fatal cancer risk from galactic cosmic rays (GCR) and solar particle events (SPE). The PDFs are used in significance tests for evaluating the effectiveness of potential radiation shielding approaches. Uncertainties in risk coefficients determined from epidemiology data, dose and dose–rate reduction factors, quality factors, and physics models of radiation environments are considered in models of cancer risk PDFs. Competing mortality risks and functional correlations in radiation quality factor uncertainties are included in the calculations. We show that the cancer risk uncertainty, defined as the ratio of the upper value of 95% confidence interval (CI) to the point estimate is about 4-fold for lunar and Mars mission risk projections. For short-stay lunar missions (), SPEs present the most significant risk, however one that is mitigated effectively by shielding, especially for carbon composites structures with high hydrogen content. In contrast, for long duration lunar () or Mars missions, GCR risks may exceed radiation risk limits that are based on acceptable levels of risk. For example, the upper 95% CI exceeding 10% fatal risk for males and females on a Mars mission. For reducing GCR cancer risks, shielding materials are marginally effective because of the penetrating nature of GCR and secondary radiation produced in tissue by relativistic particles. At the present time, polyethylene or carbon composite shielding cannot be shown to significantly reduce risk compared to aluminum shielding based on a significance test that accounts for radiobiology uncertainties in GCR risk projection.     

Photomagnetic effect in bilayer two-dimensional electron–hole systems

In tilted magnetic fields a bilayer electron–hole system is found to generate a photocurrent under terahertz radiation as the system is tuned to electron cyclotron resonance conditions. The photoinduced current amplitude oscillates with the magnetic field in correlation with Shubnikov–de Haas oscillations for electrons. The phenomenon is accounted for by a photomagnetic effect in electron–hole systems in the quantum Hall regime and has potentialities for terahertz detection and spectroscopy.     

掠入射驱动产生x射线激光的数值模拟

利用一维流体力学数值模拟程序MEDUSA和原子物理程序包，以类镍钼189nm x射线激光为例，对掠入射驱动x射线激光方案进行了研究.掠入射驱动x射线激光方案可以通过调整掠入射角来选择适合的增益区间.与正入射驱动方案相比，掠入射驱动方案加强了驱动激光在增益区内的吸收，提高了驱动激光向x射线激光的转换效率.模拟结果与实验结果符合较好. 关键词： x射线激光 掠入射辐照 激光等离子体