Nonlinear Eigenvalues for a Quasilinear Elliptic System in Orlicz–Sobolev Spaces

Using an Orlicz–Sobolev Space setting, we consider an eigenvalue problem for a system of the form

组合透镜法测量透镜焦距方法研究及数值分析

为了解决神光系列装置所需长焦透镜焦距的检测问题,在现有斐索干涉仪的基础上,对常规组合透镜方法进行了拓展,提出了双探头光栅尺法。对两种方法的工作原理及检测方法进行了分析,同时计算分析了测量数据误差对测量结果的影响,得出测量数据测量误差的上限要求。这两种方法具有测量精度高、重复性好、测量过程简单的优点,对于各类透镜焦距的检测具有重要的实用价值。     

Calixarene Dimers as Host Molecules for Biologically Important Di‐ and Oligophosphates

A dimeric calixarene, with an aliphatic C₆‐bridge and six anilinium head groups at its upper rim, preferably complexes diphosphates and oligonucleotides with more than 10 bonds between both anionic moieties. Free binding energies correlate with the length of the aliphatic bridge in a roughly linear fashion. The binding event, which is monitored by fluorescence titrations and competition experiments, relies on Coulomb interactions, as opposed to a nonpolar variant with tert‐butyl instead of ammonium groups; here, hydrophobic forces prevail, rendering the calixarene dimer selective for less polar cofactors such as FAD. The best guest for the hexaanilinium dimer is found in ssDNA, which carries multiple copies of the optimal trinucleotide for maximum attraction towards the extended cationic host. The recognition event is also observed in the environment of a lipid monolayer, and provides a means to quantify dimer diphosphate interactions by measuring p/A shifts.     

Resonance scattering spectroscopy of gold nanoparticle

The gold nanoparticles in diameter of 10-95 nm have been prepared by Frens procedure, all of which exhibit a resonance scattering peak at 580 nm. The mechanism of resonance scattering for gold nanoparticle has been considered according to the wave motion theory of nanoparticle in liquid. The principle of superamolecular interface energy band(SIEB) has been set up and utilized to explain the relationship between the diameter and colors for gold nanoparticle in liquid. A novel spectrophotometric ruler for the determination of the diameter has been proposed according to the relationship of the maximum absorption wavelength and diameter.     

港口城市形态与布局规律──以浙江省沿海港口城市为例

以浙江沿海港口城市为研究对象,通过对实地调查所取得的大量具体资料的分析,系统地探讨了浙江沿海港口城市发展的区域背景条件、优势条件和制约因素,分析了浙江沿海港口城市总体布局特征,内部结构形态和外部形态的演变发展规律,提出了浙江沿海港口城市形态与布局变化趋势,为港口城市进一步发展提供理论依据．     

Study of Tea Digitized Chromatographic Fingerprint Spectra Using Micellar Electrokinetic Chromatography

IntroductionTeaisthemostwidelyconsumedbeverageinpeople’slife .Theheightenedpopularityofthisbeveragethroughouttheworldinrecentyearsmaybedueinparttotheevidenceofarelationshipbetweenteaconsumptionandpreventionofcertainformsofhumandisease .Themaincomponentsofteaarepolyphenoliccompounds ,commonlyknownascatechins ,whichrepresentagroupofcom poundsbelongingtotheflavonoidfamily .Thesecom poundsarewidelydistributedinthetealeavesandconsti tuteupto 30 %ofthedryleafweight.1Muchinteresthasbeenfocusedoncat…     

The short ruler on cones

Abstract

On complete Riemannian manifolds, a geodesic linking two different points could be approximated by applying short ruler methods to shorten a given path iteratively. In this paper we take a closer look at a short ruler method on a cone. To handle the problems caused by the fact that the cone is not smooth at its apex, we unwind the cone isometrically into the plane, and show that the sequence of shortened curves converges to a geodesic.     

不同结构绝对光栅尺的误码机制研究

针对光栅尺具有断电位置复位、无累计误差、高精度优点,在光学隔振平台上分别建立开放式和封闭式绝对光栅尺实验系统,绝对光栅尺采用图像识别原理,以气浮直线电机ArotechABL1500为参考对象,使用激光干涉仪RENISHAW XL-80校核精度,研究不同结构绝对光栅尺的误码特点及原因。通过对比实验及研究分析,表明封闭式绝对尺相对于开放式绝对尺的误码率要高,开放式绝对式光栅尺的误码率为3%,封闭式绝对式光栅尺的误码率为8%。     

A new cosmological probe using super-massive black hole shadows

We study the prospects of using the low-redshift and high-redshift black hole shadows as new cosmological standard rulers for measuring cosmological parameters.We show that,using the low-redshift observation of the black hole shadow of M87?,the Hubble constant can be independently determined with a precision of about 13%as H0=70±9 km s?1 Mpc?1.The high-redshift observations of super-massive black hole shadows may accurately determine a combination of parameters H0 andΩm,and we show by a simple simulation that combining them with the type Ia supernovae observations would give precise measurements of the cosmological parameters.