Add to ORKGGeneralized, or power-law, inflation is shown to necessarily exist for a simple, anisotropic (Bianchi Type I) cosmology in the Einstein-Cartan gravitational theory with the Ray-Smalley (RS) improved energy-momentum tensor with spin. Formal solution of the EC field equations with the fluid equations of motion explicitly shows inflation caused by the RS spin angular kinetic energy density
Density linear perturbations in Einstein-Cartan two fluid cosmologies where the outer model is an is...
For simple inflationary models, we provide a consistent and complete scheme by which the macro-physi...
We prove the cosmic no-hair conjecture in the Einstein-Cartan theory by taking into account the effe...
Generalized, or power-law, inflation is shown to necessarily exist for a simple, anisotropic, (Bianc...
We show that the already known Bianchi type-I cosmological solutions of the self-consistent Einstein...
We develop the average effective energy-momentum tensor for a spherically symmetric cosmology with r...
The physical implications of the Raychaudhuri equation for a spinning fluid in a Riemann-Cartan spac...
Abstract. We develop the average effective energy-momentum tensor for a spherically symmelric cosmol...
In the Poincaré gauge theory of gravity, in addition to the mass-energy content, spin is also a sour...
We consider self-consistent spinning fluid cosmologies in both general relativity in Riemannian spac...
A combined BCDE (Brans-Dicke and Einstein-Cartan) theory is developed through Raychaudhuri's equatio...
Inflationary scenario has been very successful in solving various problems associated with the stand...
Analytic solutions of a particular anisotropic Bianchi type-V cosmological model with spin matter ha...
The possibility of having inflation in a renormalizable cosmological model is investigated. The Cosm...
Within the framework of the Einstein-Cartan theory a Weyssenhoff-spinuing-fluid-filled homogeneous a...
Density linear perturbations in Einstein-Cartan two fluid cosmologies where the outer model is an is...
For simple inflationary models, we provide a consistent and complete scheme by which the macro-physi...
We prove the cosmic no-hair conjecture in the Einstein-Cartan theory by taking into account the effe...
Generalized, or power-law, inflation is shown to necessarily exist for a simple, anisotropic, (Bianc...
We show that the already known Bianchi type-I cosmological solutions of the self-consistent Einstein...
We develop the average effective energy-momentum tensor for a spherically symmetric cosmology with r...
The physical implications of the Raychaudhuri equation for a spinning fluid in a Riemann-Cartan spac...
Abstract. We develop the average effective energy-momentum tensor for a spherically symmelric cosmol...
In the Poincaré gauge theory of gravity, in addition to the mass-energy content, spin is also a sour...
We consider self-consistent spinning fluid cosmologies in both general relativity in Riemannian spac...
A combined BCDE (Brans-Dicke and Einstein-Cartan) theory is developed through Raychaudhuri's equatio...
Inflationary scenario has been very successful in solving various problems associated with the stand...
Analytic solutions of a particular anisotropic Bianchi type-V cosmological model with spin matter ha...
The possibility of having inflation in a renormalizable cosmological model is investigated. The Cosm...
Within the framework of the Einstein-Cartan theory a Weyssenhoff-spinuing-fluid-filled homogeneous a...
Density linear perturbations in Einstein-Cartan two fluid cosmologies where the outer model is an is...
For simple inflationary models, we provide a consistent and complete scheme by which the macro-physi...
We prove the cosmic no-hair conjecture in the Einstein-Cartan theory by taking into account the effe...