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Nonlinear Spinor Field in Anisotropic Universes

2002/07/04 by Bijan Saha, Saha, Bijan
Earth and Planetary Sciences · Physics and Astronomy · #Cosmology and Gravitation Theories #FOS: Physical sciences #General Relativity and Quantum Cosmology (gr-qc) #Geophysics and Gravity Measurements #Relativity and Gravitational Theory #gr-qc

paper · pdf · doi:10.48550/arxiv.gr-qc/0207025

RevTex, 12 pages; Talk, given at the International Conference ``Scientific Reading devoted to 90 years anniversary of Professor Yakov Petrovich Terletski''July 1-3, 2002, Russian Peoples' Friendship University, Moscow, Russia

arxiv created 2002/07/04 · openalex publication_date 2002/07/04 · arxiv updated 2009/11/30 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28

Abstract

Evolution of an anisotropic universe described by a Bianchi type I (BI) model in presence of nonlinear spinor field has been studied by us recently in a series of papers. On offer the Bianchi models, those are both inhomogeneous and anisotropic. Within the scope of Bianchi type VI (BVI) model the self-consistent system of nonlinear spinor and gravitational fields are considered. The role of inhomogeneity in the evolution of spinor and gravitational field is studied.

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