New Perspectives in Physics from Administrator's blog

The Unified Reality Theory I: The Relational-Matrix Model (by Steven E. Kaufman): Abstract: Our modeling of space-time as a structure must include an analysis and description of these two complementary aspects, i.e., something that exists, and the way that something is arranged into a structure. What space-time is made of we will analyze and describe in terms of spatial content. This description will leave us with a model of space-time as a dynamic structure. For reasons that will later become clear, we will call this model the relational-matrix model. Once the relational-matrix model has been developed, we will then demonstrate in the future how the functioning of this dynamic spatial structure can account for certain basic aspects of the nature and behavior of physical reality.

Nonlinear Theory of Elementary Particles Part X: The Theory of Massive Neutrino (by Alexander G. Kyriakos): Abstract: In this article the theory of massive neutrino is presented. This theory does not contradict with the last data of neutrino experiments, as the Standard Model theory. The neutrino of this theory is a massive neutral particle with half spin; all neutrinos are left-handed only and all antineutrinos are right-handed only. In the theory it is shown that neutrino is not the Majorano particle, but the Dirac particle. The total lepton number is strictly conserved. The total lepton flavour numbers can not be conserved.

The Motion of Test Particle in Z = (t/z) - Type Plane Gravitational Waves in Plane Symmetry (by Sanjay R. Bhoyar, V. R. Chirde, S. D. Katore, A. G. Deshmukh): Abstract: In this paper, we have consider the plane symmetric space-time deduced by Bhoyar and Deshmukh [8] and derived the equations governing the test particle motion in the field of Z = (t/z) - type plane gravitational waves and the motion is discussed.

Bianchi Type III Magnetized Anisotropic Dark Energy Models with Constant Deceleration Parameter (by S. D. Tade, Manish M. Sambhe): Abstract: The Bianchi type III magnetized dark energy model with constant deceleration parameter is investigated. The energy-momentum tensor consists of anisotropic fluid with anisotropic EoS p = ωρ and a uniform magnetic field of energy density ρB.We obtain exact solutions to the field equations using the condition that expansion is proportional to the shear scalar . The physical behavior of the model is discussed with and without magnetic field. We conclude that universe model as well as anisotropic fluid does not approach isotropy through the evolution of the universe. The physical aspects of the dark energy models are discussed.

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