The Magnetized Universe

On the Formation of Plasma Structures in our Magnetized Dusty Universe

Our universe is magnetized and its constituents are the electrons, anti-electrons (positrons), ions and dust particles. Our objective here is to discuss the formation of large scale plasma structures based on a model associated with the Jeans instability in a self-gravitating multi-component fully ionized magnetoplasma. Assuming that the plasma particles are magnetized and charged dust grains f...

The study of Hydrodynamical wind on the observational properties of magnetized accretion flow with thermal conduction

Magnesium-iron bimetal oxides as an effective magnetized solid-base catalyst for the synthesis of substituted 2-aminthiophenes

< p>Mg-Fe bi-metal oxide was prepared and utilized as a magnetized renewable solid base catalyst for formation of 2-aminothiophenes by means of Gewald’s reaction. The prepared heterogeneous basic solid catalyst can be separated by a magnet and reused without considerable wastage in this activity. The structure of the aforementioned magnetized basic nano-catalyst was studied by XRD (X-ray diffra...

Moisturizing effects of solid lipid nanoparticles (SLN) and nanostructured lipid carriers (NLC) using deionized and magnetized water by in vivo and in vitro methods

Objective(s): The present study aimed to determine and compare moisturizing and occlusion effects of different solid lipid nanoparticles (SLN) and nanostructured lipid carriers (NLC) using magnetized water and deionized water.Materials and Methods: SLN formulations were prepared using various lipids, including Tripalmitin, Compritol®, Pr...

Magnetic Relaxation in the Bianchi-i Universe

Extended Einstein-Maxwell model and its application to the problem of evolution of magnetized Bianchi-I Universe are considered. The evolution of medium magnetization is governed by a relaxation type extended constitutive equation. The series of exact solutions to the extended master equations is obtained and discussed. The anisotropic expansion of the Bianchi-I Universe is shown to become non-...

30TH INTERNATIONAL COSMIC RAY CONFERENCE Propagation of UHE protons through a magnetized large scale structure

The propagation of UHECRs is affected by the intergalactic magnetic fields that were produced during the course of the large scale structure formation of the universe. We adopt a novel model where the large scale extragalactic magnetic fields (EGMF) are estimated from local dynamic properties of the gas flows in hydrodynamic simulations of a concordance ΛCDM universe. With the model magnetic fi...