Spinor model of a perfect fluid and their applications in Bianchi type-I and FRW models

Abstract

Different characteristic of matter influencing the evolution of the Universe has been simulated by means of a nonlinear spinor field. Exploiting the spinor description of perfect fluid and dark energy evolution of the Universe given by an anisotropic Bianchi type-I (BI) or isotropic Friedmann-Robertson-Walker (FRW) one has been studied.

10 pages, 8 Figures

References in corpus (11)

• Bouncing Universe with Quintom Matter
• Dark Energy Model with Spinor Matter and Its Quintom Scenario
• Noether symmetry for non-minimally coupled fermion fields
• Parametrization of Tachyon Field
• Proper Matter Collineations of Plane Symmetric Spacetimes
• Spinor field and accelerated regimes in cosmology
• Spinor model of a perfect fluid
• Spinor model of a perfect fluid: examples
• Scalar-Tensor Dark Energy Models
• Phantom Dark Energy and its Cosmological Consequences
• Low energy transfer cross-section for Borromean halo nuclei

Cited by in corpus (11)

• On the hadron mass decomposition
• Nonlinear Spinor Fields and its role in Cosmology
• Nonlinear Spinor Fields in Bianchi type-I spacetime: Problems and Possibilities
• Nonlinear Spinor field in isotropic space-time and dark energy models
• Dirac field as a source of the inflation in 2+1 dimensional Teleparallel gravity
• Nonlinear Spinor Fields in Bianchi type-I spacetime reexamined
• Reconstruction of f-essence and fermionic Chaplygin gas models of dark energy
• Nonlinear Spinor Fields in Bianchi type-VI spacetime
• Nonlinear Spinor Fields in Bianchi type-III spacetime
• Spinor field in Bianchi type-$IX$ space-time
• Nonlinear Spinor Fields in LRS Bianchi type-I spacetime: Theory and observation