Isotropic Spherical(各向同性球形)研究综述
Isotropic Spherical 各向同性球形 - The method is applied to calculation of fields around isolated anisotropic spherical and cylindrical inclusions in an anisotropic homogeneous host medium. [1] The main focus of this paper is to explore the possibility of providing a new family of exact solutions for suitable anisotropic spherically symmetric systems in the realm of general relativity involving the embedding spherically symmetric static metric into the five-dimensional pseudo-Euclidean space. [2] In this study, we are interested to investigate the dissipative gravitational collapse of anisotropic spherically symmetric radiating star, which satisfies the initially static Karmarkar condition in f ( R , T ) gravity. [3] In this connection, we derived the Einstein field equations for static anisotropic spherically symmetric spacetime in the mechanism of Karmakar condition. [4] The objective of the present paper is to explore and study an anisotropic spherically symmetric core-envelope model of a super dense star in which core is outfitted with linear equation of state whereas the envelope is considered to be of quadratic equation of state. [5] In this paper, we study the physical characteristics of anisotropic spherically symmetric quark star candidates for $R+2\sigma T$ gravity model, where $R$, $\sigma$ and $T$ depict scalar curvature, coupling parameter, and the trace of the energy-momentum tensor, respectively. [6] We here developed the model by considering an anisotropic spherically symmetric static general relativistic configuration that plays a significant effect on the structure and properties of stellar objects. [7] The aim of the present paper is to study an anisotropic spherically symmetric core-envelope model of a super dense star in which core is equipped with linear equation of state, consistent with the quark matter while the envelope is considered to be of quadratic equation of state by adopting the philosophy of Takisa et al. [8]该方法适用于计算各向异性均质主介质中孤立的各向异性球形和圆柱形夹杂物周围的场。 [1] 本文的主要重点是探索为广义相对论领域中合适的各向异性球对称系统提供一组新的精确解的可能性，包括将球对称静态度量嵌入到五维伪欧几里得空间中。 [2] 在这项研究中，我们有兴趣研究各向异性球对称辐射星的耗散引力坍缩，它满足 f ( R , T ) 引力中的初始静态 Karmarkar 条件。 [3] 在这方面，我们推导出了在 Karmakar 条件机制下静态各向异性球对称时空的爱因斯坦场方程。 [4] 本论文的目的是探索和研究超致密恒星的各向异性球对称核-包络模型，其中核配备线性状态方程，而包络被认为是二次状态方程。 [5] 在本文中，我们研究了$R+2\sigma T$引力模型各向异性球对称夸克星候选的物理特性，其中$R$、$\sigma$和$T$描述了标量曲率、耦合参数和分别为能量动量张量的迹线。 [6] 我们在这里通过考虑对恒星物体的结构和性质产生重大影响的各向异性球对称静态广义相对论配置来开发该模型。 [7] 本文的目的是研究超致密恒星的各向异性球对称核-包络模型，该模型的核具有与夸克物质一致的线性状态方程，而包络被认为是二次状态方程。通过采用 Takisa 等人的哲学。 [8]
isotropic spherical shell 各向同性球壳
In this study, we propose a fast approach for acoustic source localization on thin isotropic and anisotropic spherical shells. [1] The results presented agree closely with the reference results for isotropic spherical shells of revolution. [2] Acoustic source localization (ASL) on a thin isotropic spherical shell is more challenging than that for two-dimensional flat plate structures. [3] The study of stress-stain state in the isotropic spherical shells is presented in the work. [4] Considered is the stress state of an isotropic spherical shell exposed to an arbitrary load based on a non-classical theory. [5]在这项研究中，我们提出了一种在薄各向同性和各向异性球壳上进行声源定位的快速方法。 [1] 所呈现的结果与各向同性旋转球壳的参考结果非常吻合。 [2] 薄各向同性球壳上的声源定位 (ASL) 比二维平板结构更具挑战性。 [3] 工作中介绍了各向同性球壳中应力-染色状态的研究。 [4] 考虑的是基于非经典理论暴露于任意载荷下的各向同性球壳的应力状态。 [5]
isotropic spherical solution 各向同性球形溶液
We present a new systematic approach to find the exact gravitationally decoupled anisotropic spherical solution in the presence of electric charge by using the complete geometric deformation (CGD) methodology. [1] •Exact charged anisotropic spherical solutions are studied through decoupling technique. [2] Here, we present the anisotropic spherical solution in f(R, T) gravity by adopting MGD approach. [3] The aim of this paper is to obtain analytic anisotropic spherical solutions in f ( R ) scenario through gravitationally decoupled minimal geometric deformation technique. [4]我们提出了一种新的系统方法，通过使用完全几何变形 (CGD) 方法，在存在电荷的情况下找到精确的重力解耦各向异性球面解。 [1] •通过解耦技术研究了精确的带电各向异性球形溶液。 [2] 在这里，我们采用MGD方法提出了f（R，T）重力的各向异性球面解。 [3] 本文的目的是通过引力解耦最小几何变形技术获得f(R)场景下的解析各向异性球面解。 [4]
isotropic spherical semivariogram
An Isotropic Spherical semivariogram model was fitted on the residuals and a simple residual Kriging was executed in which the error obtained was -0. [1] Isotropic spherical semivariogram models were fitted using the least squares method, and they showed a pattern of spatial dependence for all years. [2]对残差拟合各向同性球形半变异函数模型，并执行简单的残差克里金法，其中获得的误差为 -0。 [1] 使用最小二乘法拟合各向同性球面半变异函数模型，它们显示出所有年份的空间依赖性模式。 [2]
isotropic spherical particle
We also detect the rotation with our newly developed pitch rotational motion detection technique which could not be done conventionally on isotropic spherical particles. [1] 1 Licensing provisions: GPLv3 Programming language: MATLAB Nature of problem: Decomposition of optical force acting on an isotropic spherical particle of size comparable to optical wave length into conservative (gradient) and nonconservative (scattering) components. [2]我们还使用我们新开发的俯仰旋转运动检测技术来检测旋转，这在传统的各向同性球形粒子上是无法做到的。 [1] 1 许可规定：GPLv3 编程语言：MATLAB 问题性质：将作用于尺寸与光波长相当的各向同性球形粒子上的光力分解为保守（梯度）和非保守（散射）分量。 [2]