Introduction to Isotropic Spherical

The method is applied to calculation of fields around isolated anisotropic spherical and cylindrical inclusions in an anisotropic homogeneous host medium.

We also detect the rotation with our newly developed pitch rotational motion detection technique which could not be done conventionally on isotropic spherical particles.

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.

In this study, we propose a fast approach for acoustic source localization on thin isotropic and anisotropic spherical shells.

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.

The results presented agree closely with the reference results for isotropic spherical shells of revolution.

•Exact charged anisotropic spherical solutions are studied through decoupling technique.

Acoustic source localization (ASL) on a thin isotropic spherical shell is more challenging than that for two-dimensional flat plate structures.

So far, most studies have considered isotropic spherical tracer particles, while the diffusion of anisotropic particles has rarely been involved.

We conclude that the secular relaxation of hot isotropic spherical clusters is not dominated by collectively amplified large-scale potential fluctuations, despite the existence of a strong ℓ = 1 damped mode.

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.

The permeability is increased sharply once deviating the isotropic spherical stress state, but it is no longer changed obviously after the lateral coefficient has been increased or decreased more than 20%.

This review tries to provide a general perspective of the physico-chemical aspects associated with the stabilization of interfaces by colloidal particles, mainly chemical isotropic spherical colloids.

The study of stress-stain state in the isotropic spherical shells is presented in the work.

In this connection, we derived the Einstein field equations for static anisotropic spherically symmetric spacetime in the mechanism of Karmakar condition.

Here, we present the anisotropic spherical solution in f(R, T) gravity by adopting MGD approach.

Refined microstructural parameters were obtained using the anisotropic spherical harmonic size approach and correlated with the above estimation methods and transmission electron microscopy images.

An Isotropic Spherical semivariogram model was fitted on the residuals and a simple residual Kriging was executed in which the error obtained was -0.

Isotropic spherical semivariogram models were fitted using the least squares method, and they showed a pattern of spatial dependence for all years.

Considered is the stress state of an isotropic spherical shell exposed to an arbitrary load based on a non-classical theory.

Slower surface crystallization kinetics, higher surface glass transition temperature (Tgsurface), and suppressed Tg-confinement effect were observed when the surface average conformation changed from oriented oblate ellipsoidal conformation to isotropic spherical conformation, showing that surface dynamics is very sensitive to chain conformation.

In this research paper, we address the issues of expansion and gravitational collapse of anisotropic spherical source in the presence of cosmological constant.

In this paper, we investigate the effects of electromagnetic field on the isotropic spherical gravastar models in metric $f(R,T)$ gravity.

The aim of this paper is to obtain analytic anisotropic spherical solutions in f ( R ) scenario through gravitationally decoupled minimal geometric deformation technique.

Unexpectedly, an interesting anisotropic needle-like rather than an ordinary isotropic spherical supramolecular amphiphilic assembly was fabricated by the complexation of calixpyridinium with methotrexate disodium.

First, longitudinal-to-longitudinal backscattering amplitudes from single grains are predicted, where the setup and configuration of the finite element (FE) model are verified with an isotropic spherical inclusion for which an exact solution is available.

Here we biosynthesized monodispersed isotropic and polydispersed anisotropic spherical AuNPs from leaf and seed extract broths of the medicinal plant Peganum harmala L.

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.

The isotropic spherical giant-shell nanocrystals show consistently stronger exciton-phonon coupling as compared to the anisotropic rod-shaped dot-in-rod (DiR) architecture, and the 2LO/LO intensity ratio decreases for excitation wavelengths approaching the CdS band edge.

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.

The human’s visual field is modeled as an anisotropic spherical sensor, which decays in acuity towards the periphery, and is integrated in time throughout the domain.

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.

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.

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.