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Calculate central limit theorem for the number of empty cells after allocation of particles 计算分配粒子后空细胞数的中心极限定理
Q4 MATHEMATICS Pub Date : 2021-12-19 DOI: 10.21744/ijpm.v5n1.1803
O. A. Islamova, Z. S. Chay, F. S. Rakhimova, Feruza Abdullayeva
This work belongs to the field of limit theorems for separable statistics. In particular, this paper considers the number of empty cells after placing particles in a finite number of cells, where each particle is placed in a polynomial scheme. The statistics under consideration belong to the class of separable statistics, which were previously considered in (Mirakhmedov: 1985), where necessary statements for the layout of particles in a countable number of cells were proved. The same scheme was considered in (Asimov: 1982), in which the conditions for the asymptotic normality of random variables were established. In this paper, the asymptotic normality of the statistics in question is proved and an estimate of the remainder term in the central limit theorem is obtained. In summary, the demand for separable statistics systems is growing day by day to address large-scale databases or to facilitate user access to data management. Because such systems are not only used for data entry and storage, they also describe their structure: file collection supports logical consistency; provides data processing language; restores data after various interruptions; database management systems allow multiple users.
本工作属于可分离统计量的极限定理领域。特别地,本文考虑在有限数量的单元格中放置粒子后的空单元格数,其中每个粒子以多项式格式放置。所考虑的统计量属于可分离统计量的类别,这是先前在(Mirakhmedov: 1985)中考虑过的,在那里证明了在可数细胞中粒子布局的必要陈述。在(Asimov: 1982)中考虑了相同的方案,其中建立了随机变量的渐近正态性的条件。本文证明了所讨论的统计量的渐近正态性,并给出了中心极限定理中剩余项的一个估计。总之,对可分离统计系统的需求日益增长,以解决大规模数据库或方便用户访问数据管理。因为这样的系统不仅用于数据输入和存储,它们还描述了它们的结构:文件收集支持逻辑一致性;提供数据处理语言;在各种中断后恢复数据;数据库管理系统允许多个用户。
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引用次数: 1
Gas Dynamics type Burgers equation with convolutional nonlinearity 具有卷积非线性的气体动力学Burgers方程
Q4 MATHEMATICS Pub Date : 2021-12-01 DOI: 10.26577/ijmph.2021.v12.i2.01
D. Serikbaev
In this paper, we consider an initial value problem for the Burgers’ equation with convolution type weak nonlinearity for the Sturm–Liouville operator. We prove that this problem has an explicit solution in the form of series. To achieve our goals, we use methods that correspond to various fields of mathematics, such as the theory of partial differential equations, mathematical physics, and functional analysis. In particular, we use the Fourier analysis method to establish the existence of solutions to this problem on the Sobolev space. As far as we know, it is the first result obtained for the convolution type Burgers’ equation. Since, we use the Fourier analysis method we gave the properties of Fourier transform when acting on convolution, and also gave a property of fractional order of the Sturm–Liouville operator. The generalized solutions of the convolution type weak nonlinear Burgers’ equation with the initial Cauchy condition are studied.
本文研究了一类具有Sturm-Liouville算子的弱非线性卷积型Burgers方程的初值问题。证明了该问题具有级数形式的显式解。为了实现我们的目标,我们使用了与数学各个领域相对应的方法,例如偏微分方程理论、数学物理和泛函分析。特别地,我们用傅里叶分析方法在Sobolev空间上证明了该问题解的存在性。据我们所知,这是卷积型Burgers方程得到的第一个结果。由于我们使用傅里叶分析方法,我们给出了傅里叶变换作用于卷积时的性质,同时也给出了Sturm-Liouville算子的分数阶性质。研究了具有初始柯西条件的卷积型弱非线性Burgers方程的广义解。
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引用次数: 0
Similarity solution of two-phase cylindrical Stefan solidification problem 两相圆柱形Stefan凝固问题的相似解
Q4 MATHEMATICS Pub Date : 2021-12-01 DOI: 10.26577/ijmph.2021.v12.i2.03
T. Nauryz
The mathematical model of determining temperature fields in cylindrical domain with solidification process is represented. The solidification process of cylinder due to cooling is constructed by two-phase cylindrical Stefan problem for liquid and solid zones with freezing interface. Respect to strength of the heat sink at the center of cylindrical material boundary condition 1 0 0 lim[2 ] r r r         is an important to determine temperature in solid domain. The analytical solution of the problem is introduced with method of similarity principle which enables us to reduce free boundary problem to ordinary differential equations. Temperature solutions of solid and liquid zones are represented by special function which called exponential integral equation. The free boundary at freezing interface and temperatures at two phases are determined. Lemmas about exponential integral functions are introduced and used to prove that obtained operator function is contraction operator. Upper boundness of the exponential integral function is checked graphically. It is shown that existence of uniqueness of solution exists.
建立了凝固过程中柱面温度场确定的数学模型。采用两相圆柱形Stefan问题,构建了具有冻结界面的液固两区圆柱体冷却凝固过程。对散热器的圆柱的中心物质边界条件1 0 0 lim [2] r r r温度是一个重要的决定在固体域。用相似原理的方法给出了该问题的解析解,使我们能够将自由边界问题化为常微分方程。固体和液体区域的温度解用指数积分方程表示。确定了冻结界面的自由边界和两相温度。引入指数积分函数的引理,并利用引理证明所得到的算子函数是收缩算子。用图形法检验了指数积分函数的上界。证明了解的唯一性的存在性。
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引用次数: 0
Motion of stars near the galactic center 星系中心附近恒星的运动
Q4 MATHEMATICS Pub Date : 2021-12-01 DOI: 10.26577/ijmph.2021.v12.i2.09
K. Boshkayev, T. Konysbayev, E. Kurmanov, O. Luongo, M. Muccino, H. Quevedo, A. Taukenova, A. Urazalina, G. Zhumakhanova
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引用次数: 0
ZnO nanowires for photoelectric converter applications 光电变换器用ZnO纳米线
Q4 MATHEMATICS Pub Date : 2021-12-01 DOI: 10.26577/ijmph.2021.v12.i2.08
V. Kidalov, N. Sosnytska, A. Dyadenchuk, R. Oleksenko
This work is focused on the creation and study of photosensitive structures based on zinc oxide nanofibers, which are promising for solar energy. Zinc oxide nanowires were obtained on the porous zinc selenide surface. The porous substrate was obtained by electrochemical etching of a low-resistance n-ZnSe plate (110) with a polished surface. Nanowires were deposited by radical-beam epitaxy. The annealing temperature was varied from 400° C to 500° C. The oxygen radical flux was 1.5∙1017 cm-2s-1. The process duration was 50 minutes. According to the scanning electron microscopy results, the nanowires length reaches 10 μm, the nanowires diameter is ~1 μm. The predominant X-ray diffraction reflex at 2θ=34.44° indicates the polycrystalline nature of the manufactured ZnO coatings with a wurtzite-type hexagonal lattice. The study of nanowires ZnO luminescence at room temperature contains an ultraviolet peak around 385 nm. This peak is related to the zinc oxide edge luminescence. Based on the fabricated structure, the design of the photoconverter was developed. The upper contact of the fabricated photoelectric converter was created by vacuum thermal sputtering of aluminum through a mask. The deposition was carried out at a substrate temperature of 200° C. Ohmic contacts were made using conductive silver paste. The reverse ohmic contact was formed by applying Al paste to the entire reverse side of the surface. The upper layer of the structure is an array of ZnO nanowires. The active base layer is ZnSe. The light volt-ampere characteristics of the obtained structure were measured in the AM 1.5 illumination mode. No-load voltage Uxx, short-circuit current Isc and the fill factor of the current-voltage characteristic FF of the solar element were measured. The efficiency of the manufactured photoconverter was 13.7 %.
本文主要研究了基于氧化锌纳米纤维的光敏结构材料,该材料在太阳能领域具有广阔的应用前景。在多孔硒化锌表面制备了氧化锌纳米线。通过电化学刻蚀表面抛光的低电阻n-ZnSe板(110)得到多孔衬底。采用自由基束外延法制备纳米线。退火温度为400℃~ 500℃,氧自由基通量为1.5∙1017 cm-2s-1。进程持续时间为50分钟。扫描电镜结果显示,纳米线长度达到10 μm,纳米线直径为~1 μm。在2θ=34.44°处的主要x射线衍射反射表明制备的ZnO涂层具有纤锌矿型六边形晶格的多晶性质。纳米线ZnO在室温下的发光包含一个约385 nm的紫外峰。此峰与氧化锌边缘发光有关。在此基础上,进行了光电变换器的设计。所制备的光电转换器的上接点是通过掩模对铝进行真空热溅射形成的。在200℃的衬底温度下进行沉积,欧姆接触采用导电银膏。反向欧姆接触是通过在整个表面的背面涂铝膏形成的。该结构的上层是ZnO纳米线阵列。活性基础层为ZnSe。在AM 1.5照明模式下测量了所得结构的光伏安特性。测量了太阳能元件的空载电压Uxx、短路电流Isc和电流电压特性FF的填充系数。该光电转换器的效率为13.7%。
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引用次数: 1
An Interpolated Bounce Back Thermable Method for Simulating Solid Particles Dynamics in a Viscous Medium 粘性介质中固体粒子动力学模拟的插值弹回热方法
Q4 MATHEMATICS Pub Date : 2021-12-01 DOI: 10.26577/ijmph.2021.v12.i2.06
D. Zhakebayev, A. Zhumali, B. Satenova
In this paper we discuss the mathematical and computer modeling of non-isothermal two-phase flows with suspended particles. Natural convection between an outer cubical cavity and an inner hot sphere is investigated. To simulate heat fluxes loaded with particles, a thermal model of the lattice Boltzmann equation in combination with the interpolated bounce back method (TLBM-IBB) has been developed. In TLBM-IBB, IBB is used to process liquid-solid interfaces, and TLBM is used to simulate the heat flow of a fluid. The momentum exchange method is used to calculate the hydrodynamic force on the particle surface. Simulation performed for a range of Rayleigh numbers . The accuracy and efficiency of the existing method is demonstrated by the example of solving the test problem of natural convection around a stationary particle and three-dimensional compressible natural convection in a square cavity filled with air, which has a hot wall on the left and a cold wall on the right, and two horizontal walls are adiabatic. The results obtained are in good agreement with the experimental and numerical results of other authors.
本文讨论了含悬浮颗粒的非等温两相流的数学和计算机建模。研究了外部立方体空腔和内部热球之间的自然对流。为了模拟粒子负载的热通量,结合插值反弹法(TLBM-IBB)建立了晶格玻尔兹曼方程的热模型。在TLBM-IBB中,IBB用于处理液固界面,TLBM用于模拟流体的热流。动量交换法用于计算颗粒表面的流体动力。对一系列瑞利数进行的模拟。通过求解静止粒子周围的自然对流和填充空气的方形空腔中的三维可压缩自然对流的测试问题的例子,证明了现有方法的准确性和有效性。方形空腔左有热壁,右有冷壁,两个水平壁是绝热的。所得结果与其他作者的实验和数值结果吻合良好。
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引用次数: 0
On one integrable cosmological model of the flat universe in k-essence 关于k本质中平坦宇宙的一个可积宇宙学模型
Q4 MATHEMATICS Pub Date : 2021-12-01 DOI: 10.26577/ijmph.2021.v12.i2.010
K. Myrzakulov, D. Kenzhalin, T. Myrzakul
. The study of the origin and evolution of our Universe is one of the interesting and actual directions in modern physics and astrophysics. This paper considers the cosmological model of the Universe in the Einstein's theory of gravity and k -essence, where the gravitational field interacts in a non-minimal way with the scalar field φ . That is, in action, in the role of the matter field, we consider the special case of the Lagrange function for the essence. The corresponding field equations of the considered model are obtained. Also, particular solutions for the scale factor a ( t ) were obtained in the form of de Sitter's solution. Two solutions were found, for the potential energy V ( t ) and the scalar field φ ( t ), and their graphical solutions were also built. The analytical solutions obtained in this work are solutions of the considered integrable systems. These solutions are in good agreement with the available observational data and are able to describe the modern dynamics of the expansion of the Universe.
. 研究宇宙的起源和演化是现代物理学和天体物理学中有趣而实际的方向之一。本文考虑了爱因斯坦引力和k -本质理论中引力场与标量场φ以非极小方式相互作用的宇宙模型。也就是说,在作用中,在物质场的作用下,我们考虑以拉格朗日函数为本质的特殊情况。得到了所考虑模型的相应场方程。并以德西特解的形式得到了尺度因子a (t)的特解。得到了势能V (t)和标量场φ (t)的两个解,并建立了它们的图形解。本文所得到的解析解是所考虑的可积系统的解。这些解与现有的观测数据非常吻合,能够描述宇宙膨胀的现代动力学。
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引用次数: 0
Control of Vibrations of a Beam with Nonlocal Boundary Conditions 具有非局部边界条件的梁的振动控制
Q4 MATHEMATICS Pub Date : 2021-12-01 DOI: 10.26577/ijmph.2021.v12.i2.05
D. Nurakhmetov, S. Jumabayev, A. Aniyarov
In this article is considered the models of uniform Euler-Bernoulli beams with an arbitrary variable coefficient of foundation on a finite segment. The variable of foundation corresponds to the Winkler model. The control problem the first eigenvalues of the beam vibration is investigated. Two types of fastenings at the ends are considered: clamped-clamped and hinged-hinged. The control is based on the Kanguzhin algorithm through integral perturbations of one of the boundary conditions of the original problem. Conditions for the boundary parameters for controlling the first eigenvalues are found. First, a result is formulated regarding the control of the first eigenvalue of the oscillation of the Euler-Bernoulli beam with hinge fastening at both ends. The result is then extended to control with several eigenvalues for this beam, which are important from the point of view of the application. Such questions are especially relevant when studying the resonant natural frequencies of a mechanical system. A similar result was obtained for a Euler-Bernoulli beam with clamped fastening at both ends. Such results of eigenvalue control of a mechanical system contribute to the creation of various non-destructive testing devices that are widely used in technical acoustics.
本文研究了在有限段上具有任意变地基系数的均匀欧拉-伯努利梁的模型。基础的变量对应于Winkler模型。研究了梁振动的第一特征值控制问题。端部的紧固件有两种类型:夹紧式和铰接式。该控制基于Kanguzin算法,通过对原始问题的一个边界条件的积分扰动。找到了控制第一特征值的边界参数的条件。首先,给出了两端铰接的欧拉-伯努利梁振动第一特征值的控制结果。然后将结果推广到具有该梁的几个特征值的控制,这些特征值从应用的角度来看是重要的。当研究机械系统的共振固有频率时,这些问题尤其相关。对于两端都有夹紧紧固的欧拉-伯努利梁,也获得了类似的结果。机械系统的特征值控制的这种结果有助于创建在技术声学中广泛使用的各种无损检测设备。
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引用次数: 0
An Efficient Privacy and Integrity-Preserving Range Query Scheme over Unsorted Data in IoT Two-tiered Wireless Sensor Networks 物联网双层无线传感器网络中一种有效的基于未分类数据的隐私和完整性保护范围查询方案
Q4 MATHEMATICS Pub Date : 2021-12-01 DOI: 10.26577/ijmph.2021.v12.i2.04
Kimbugwe Nasser, Tingrui Pei
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引用次数: 1
Static and rotating white dwarf stars at finite temperatures 静止和旋转的白矮星在有限的温度下
Q4 MATHEMATICS Pub Date : 2021-12-01 DOI: 10.26577/ijmph.2021.v12.i2.07
K. Boshkayev, O. Luongo, M. Muccino, H. Quevedo
. Static and rotating, cold and hot white dwarf stars are investigated both in Newtonian gravity and general theory of relativity, employing the well-established Chandrasekhar equation of state. The Hartle formalism is involved to construct and study uniformly rotating configurations of white dwarfs. The mass-radius, mass-central density, radius-central density and other basic relations of stable white dwarfs, consisting of pure helium and iron, are constructed for different temperatures at mass shedding limit. Stability of white dwarfs is analyzed with respect to the inverse beta decay process, pycnonuclear reactions and instabilities of general relativity. It is found that for a fixed mass hot white dwarfs consisting of pure iron are smaller in size, correspondingly denser with respect to the ones composed of light elements. In addition, it is shown that near the Chandrasekhar mass limit the mass of hot rotating white dwarfs is slightly less than for cold ones, though for low mass rotating white dwarfs and static ones in all mass range the situation is opposite.
。利用公认的钱德拉塞卡状态方程,在牛顿引力和广义相对论中研究了静态和旋转、冷和热白矮星。哈特尔形式论被用于构造和研究白矮星的均匀旋转构型。建立了纯氦和纯铁组成的稳定白矮星在质量脱落极限下不同温度下的质量半径、质量中心密度、半径中心密度等基本关系。从逆衰变过程、核原子反应和广义相对论的不稳定性等方面分析了白矮星的稳定性。我们发现,对于质量固定的纯铁组成的热白矮星,其体积较小,相对于由轻元素组成的白矮星密度更大。此外,在钱德拉塞卡质量极限附近,热旋转白矮星的质量略小于冷旋转白矮星的质量,而在所有质量范围内的低质量旋转白矮星和静止白矮星的情况则相反。
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引用次数: 0
期刊
International Journal of Mathematics and Physics
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