The Experts below are selected from a list of 291 Experts worldwide ranked by ideXlab platform
Anirudh Pradhan - One of the best experts on this subject based on the ideXlab platform.
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A Plane-Symmetric Inhomogeneous Cosmological Model of Perfect Fluid Distribution with Electromagnetic Field I
Communications in Theoretical Physics, 2010Co-Authors: Anirudh Pradhan, Prashant Singh, Anil Kumar YadavAbstract:A plane-symmetric inhomogeneous cosmological model of perfect fluid distribution with electro-magnetic field is obtained. F12 is the non-vanishing component of electromagnetic field tensor. To get a Deterministic Solution, we assume the free gravitational field is Petrov type-II non-degenerate. Some physical and geometric properties of the model are also discussed.
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A New Class of String Cosmological Models in Cylindrically Symmetric Inhomogeneous Universe
Astrophysics and Space Science, 2008Co-Authors: Anil Kumar Yadav, Mukesh Kumar Mishra, Anirudh PradhanAbstract:A new class of cylindrically symmetric inhomogeneous string cosmological models is investigated. To get the Deterministic Solution, it has been assumed that the expansion ($\theta$) in the model is proportional to the eigen value $\sigma^{1}_{1}$ of the shear tensor $\sigma^{i}_{j}$. The physical and geometric aspects of the model are also discussed.
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magnetized string cosmological model in cylindrically symmetric inhomogeneous universe with time dependent cosmological term λ
Brazilian Journal of Physics, 2008Co-Authors: Anirudh Pradhan, Kanti Jotania, Archana SinghAbstract:Cylindrically symmetric inhomogeneous magnetized string cosmological model is investigated with cosmological term L varying with time. To get the Deterministic Solution, it has been assumed that the expansion (q) in the model is proportional to the eigen value s1 1 of the shear tensor si j. The value of cosmological constant for the model is found to be small and positive which is supported by the results from recent supernovae Ia observations. The physical and geometric properties of the model are also discussed in presence and absence of magnetic field.
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CYLINDRICALLY SYMMETRIC INHOMOGENEOUS UNIVERSE WITH ELECTROMAGNETIC FIELD IN STRING COSMOLOGY
Astrophysics and Space Science, 2007Co-Authors: Anirudh Pradhan, Sheel Kumar SinghAbstract:Cylindrically symmetric inhomogeneous string cosmological model in presence of electromagnetic field is investigated. We have assumed that F23 is the only non-vanishing component of Fij. To get the Deterministic Solution, it has been assumed that the expansion (θ) in the model is proportional to the eigen value σ11 of the shear tensor σij. The physical and geometric aspects of the model are also discussed.
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magnetized string cosmological model in cylindrically symmetric inhomogeneous universe with variable cosmological term lambda
arXiv: General Relativity and Quantum Cosmology, 2007Co-Authors: Anirudh PradhanAbstract:Cylindrically symmetric inhomogeneous magnetized string cosmological model is investigated with cosmological term $\Lambda$ varying with time. To get the Deterministic Solution, it has been assumed that the expansion ($\theta$) in the model is proportional to the eigenvalue $\sigma^{1}_{1}$ of the shear tensor $\sigma^{i}_{j}$. The value of cosmological constant for the model is found to be small and positive which is supported by the results from recent supernovae Ia observations. The physical and geometric properties of the model are also discussed in presence and absence of magnetic field.
Dan Jiao - One of the best experts on this subject based on the ideXlab platform.
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a Deterministic Solution based fast eigenvalue solver with guaranteed convergence for finite element based 3 d electromagnetic analysis
IEEE Transactions on Antennas and Propagation, 2013Co-Authors: Feng Sheng, Dan JiaoAbstract:A fast Solution to both the quadratic eigenvalue problem and the generalized eigenvalue problem is developed for the finite-element based analysis of general 3-D electromagnetic problems. Given an arbitrary frequency band of interest, denoting the number of physically important eigenvalues for this band by , the proposed eigenvalue Solution is capable of solving a significantly reduced eigenvalue problem of O(k) to find a complete set of eigenvalues and eigenvectors that are physically important for the given frequency band. In addition to bypassing the need of solving a large-scale eigenvalue problem of O(N), with N being the system matrix size, the reduced eigenvalue problem is constructed from O(k) Solutions to a Deterministic problem. As a result, the methods that have been developed to solve Deterministic problems and their fast solvers can all be readily leveraged to solve eigenvalue problems. Moreover, the proposed fast eigenvalue Solution has guaranteed convergence and controlled accuracy, which is theoretically proved in this paper. The Solution is applicable to general 3-D problems where the structures are arbitrary, materials are inhomogeneous, and both dielectrics and conductors can be lossy. Applications to microwave devices, package structures, and on-chip integrated circuits have demonstrated the accuracy, efficiency, and convergence of the proposed fast eigenvalue Solution.
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a Deterministic Solution based fast quadratic eigenvalue solver for 3 d finite element analysis
International Symposium on Antennas and Propagation, 2012Co-Authors: Feng Sheng, Dan JiaoAbstract:A fast Solution to the quadratic eigenvalue problem resulting from the finite element based analysis of general electromagnetic problems with lossy conductors and materials is developed. Given an arbitrary frequency band, the proposed solver is capable of solving a significantly reduced eigenvalue problem of O(k) to find a complete set of the eigenvalues and eigenvectors that are physically important for this frequency band, the number of which is k. The reduced eigenvalue problem is constructed from O(k) Solutions to a Deterministic problem. Its convergence and accuracy are theoretically proved. The proposed solver is applicable to general 3-D problems where the structures are arbitrary, materials are inhomogeneous, and both dielectrics and conductors can be lossy.
Anil Kumar Yadav - One of the best experts on this subject based on the ideXlab platform.
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A Plane-Symmetric Inhomogeneous Cosmological Model of Perfect Fluid Distribution with Electromagnetic Field I
Communications in Theoretical Physics, 2010Co-Authors: Anirudh Pradhan, Prashant Singh, Anil Kumar YadavAbstract:A plane-symmetric inhomogeneous cosmological model of perfect fluid distribution with electro-magnetic field is obtained. F12 is the non-vanishing component of electromagnetic field tensor. To get a Deterministic Solution, we assume the free gravitational field is Petrov type-II non-degenerate. Some physical and geometric properties of the model are also discussed.
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Thermodynamical Behavior of Inhomogeneous Universe with Varying Λ in Presence of Electromagnetic Field
International Journal of Theoretical Physics, 2010Co-Authors: Anil Kumar YadavAbstract:Thermodynamical behavior of inhomogeneous universe with varying Λ in presence of electromagnetic field is obtained. F12 is the non-vanishing component of electromagnetic field tensor. To get a Deterministic Solution, it is assumed that the free gravitational field is Petrov type-II non-degenerate. The value of cosmological constant is found to be small and positive supported by recent results from the supernovae observations recently obtained by High-Z Supernovae Ia Team and Supernovae Cosmological Project. A relation between cosmological constant and thermodynamical quantities is established. Some physical and geometric properties of the model are also discussed.
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A New Class of String Cosmological Models in Cylindrically Symmetric Inhomogeneous Universe
Astrophysics and Space Science, 2008Co-Authors: Anil Kumar Yadav, Mukesh Kumar Mishra, Anirudh PradhanAbstract:A new class of cylindrically symmetric inhomogeneous string cosmological models is investigated. To get the Deterministic Solution, it has been assumed that the expansion ($\theta$) in the model is proportional to the eigen value $\sigma^{1}_{1}$ of the shear tensor $\sigma^{i}_{j}$. The physical and geometric aspects of the model are also discussed.
Barkha R. Tripathi - One of the best experts on this subject based on the ideXlab platform.
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Bianchi Type-VI0 Inhomogeneous Cosmological Model for Stiff Perfect Fluid Distribution in General Relativity
Prespacetime Journal, 2017Co-Authors: Atul Tyagi, Barkha R. TripathiAbstract:In this paper, we have investigated an inhomogeneous Bianchi type VI 0 cosmological model for stiff perfect fluid distribution in general relativity. To obtain the Deterministic Solution of Einstein’s field equations, we assume that the isotropic pressure is equal to rest density i.e. p = ρ. Some physical and geometric aspects of the models are also discussed.
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Inhomogeneous Bianchi Type - I Cosmological Model For Stiff Perfect Fluid Distribution
Prespacetime Journal, 2016Co-Authors: Atul Tyagi, Swati Parikh, Barkha R. TripathiAbstract:In this paper we have investigated inhomogeneous Bianchi type I cosmological model for stiff fluid. To get the Deterministic Solution of Einstein’s field equation, we assume that the isotropic pressure is equal to energy density i.e. p = e . Various physical and geometrical properties of the model are also discussed.
Alexander Alekseenko - One of the best experts on this subject based on the ideXlab platform.
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Deterministic Solution of the spatially homogeneous boltzmann equation using discontinuous galerkin discretizations in the velocity space
Journal of Computational Physics, 2014Co-Authors: Alexander Alekseenko, E JosyulaAbstract:Abstract We present a new Deterministic approach for the Solution of the spatially homogeneous Boltzmann kinetic equation based on nodal discontinuous Galerkin (DG) discretizations in the velocity space. In the new approach the collision operator has the form of a bilinear operator with a pre-computed kernel; its evaluation requires O ( n 5 ) operations at every point of the phase space where n is the number of degrees of freedom in one velocity dimension. The method is generalized to any molecular potential. Results of numerical simulations are presented for the problem of spatially homogeneous relaxation for the hard spheres potential. Comparison with the method of Direct Simulation Monte Carlo showed excellent agreement.
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Deterministic Solution of the boltzmann equation using a discontinuous galerkin velocity discretization
28TH INTERNATIONAL SYMPOSIUM ON RAREFIED GAS DYNAMICS 2012, 2012Co-Authors: Alexander Alekseenko, E JosyulaAbstract:We propose an approach for high order discretization of the Boltzmann equation in the velocity space using discontinuous Galerkin methods. Our approach employs a reformulation of the collision integral in the form of a bilinear operator with a time-independent kernel. In the fully non-linear case the complexity of the method is O(n8) operations per spatial cell where n is the number of degrees of freedom in one velocity direction. The new method is suitable for parallelization to a large number of processors. Techniques of automatic perturbation decomposition and linearisation are developed to achieve additional performance improvement. The number of operations per spatial cell in the linearised regime is O(n6). The method is applied to the Solution of the spatially homogeneous relaxation problem. Mass momentum and energy is conserved to a good precision in the computed Solutions.