Cosmology with an Effective -Term in Lyra Manifold
arXiv:1307.1866 · doi:10.1088/0256-307X/30/11/119801
Abstract
A cosmological model in Lyra's geometry are studied under the assumption that an effective cosmological term is appeared in the field equations as the result of interaction between the displacement vector field and an auxiliary - term. Some exact solutions of the model equations are obtained and preliminary studied for the simplest cases in order to illustrate how such a model works
5 pages, 1 figure
References in corpus (7)
- Spectra and Light Curves of Six Type Ia Supernovae at 0.511 < z < 1.12 and the Union2 Compilation
- Fractional Einstein-Hilbert Action Cosmology
- Observational constraints on new generalized Chaplygin gas model
- A Dark Energy Model in Lyra Manifold
- Cosmological Models with a Varying -Term in Lyra's Geometry
- Constraints on the unified dark energy-dark matter model from latest observational data
- Comparison of Supernovae datasets Constraints on Dark Energy
Cited by in corpus (7)
- On Bianchi type III Cosmological Model with Quadratic EoS in Lyra Geometry
- Interacting Ricci dark energy models with an effective -term in Lyra manifold
- A cosmological model of the early universe based on ECG with variable -term in Lyra geometry
- Quintessence Cosmology with an Effective -Term in Lyra Manifold
- Toy models of Universe with an Effective varying -Term in Lyra Manifold
- Exact Cosmological Models with the Yang - Mills Fields on Lyra Manifold
- Behavior of vacuum and naked singularity under smooth gauge function in Lyra geometry