Magnetized string cosmological model in cylindrically symmetric inhomogeneous universe with time dependent cosmological-term lambda
AUTOR(ES)
Pradhan, Anirudh, Jotania, Kanti, Singh, Archana
FONTE
Brazilian Journal of Physics
DATA DE PUBLICAÇÃO
2008-03
RESUMO
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 eigen value sigma1 1 of the shear tensor sigmai 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.
Documentos Relacionados
- Some magnetized bianchi type-III massive string cosmological models in general relativity
- Cosmological models of universe with variable deceleration parameter in Lyra's manifold
- Steady-state polarization from cylindrically symmetric fluorophores undergoing rapid restricted motion.
- Supernovae, an accelerating universe and the cosmological constant
- Inhomogeneous basis set of symmetric polynomials defined by tableaux.