Magnetized cosmological model
- Resource Type
- Journal Article
- Authors
- Source
- Int. J. Theor. Phys.; (United States); 25:7
- Subject
- 71 CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS COSMOLOGICAL MODELS
ELECTROMAGNETIC FIELDS
FLUIDS
EIGENVALUES
ELECTRIC CONDUCTIVITY
ENERGY-MOMENTUM TENSOR
GALACTIC EVOLUTION
MAGNETIC FLUX
MAXWELL EQUATIONS
METRICS
SHEAR
SPACE-TIME
DIFFERENTIAL EQUATIONS
ELECTRICAL PROPERTIES
EQUATIONS
MATHEMATICAL MODELS
PARTIAL DIFFERENTIAL EQUATIONS
PHYSICAL PROPERTIES
TENSORS 640106* -- Astrophysics & Cosmology-- Cosmology
- Language
- English
The object of this paper is to investigate the behavior of the magnetic field in a cosmological model for perfect fluid distribution. The magnetic field is due to an electric current produced along the /chi/ axis. It is assumed that expansion (/theta/) in the model is proportional to sigma/sup 1//sub 1/, the eigenvalue of the shear tensor sigma /sup j/ /sub i/. The behavior of the model when the magnetic field tends to zero and other physical properties are also discussed.