We consider spatially homogeneous and isotropic cosmologies with non-vanishing torsion,
which assumes a specific form due to the high symmetry of these universes. Using covariant …

The Einstein static (ES) universe has played a major role in various emergent scenarios
recently proposed in order to cure the problem of the initial singularity of the standard model …

Exploring the characterization of singular black hole spacetimes, we study the relation
between energy density, curvature invariants, and geodesic completeness using a quadratic …

In the present work, we investigate wormhole structures and the energy conditions
supporting them in Einstein-Cartan theory. The matter content consists of a Weyssenhoff …

We present a historical review of Einstein's 1917 paper 'Cosmological Considerations in the
General Theory of Relativity'to mark the centenary of a key work that set the foundations of …

We reconstruct the $\Lambda $ CDM model for $ f (T,\mathcal {T}) $ Theory, where $ T $ is
the torsion scalar and $\mathcal {T} $ the trace of the energy-momentum tensor. The result …

Abstract Cosmologies based on General Relativity encompassing an anti-symmetric
connection (torsion) can display nice desirable features as the absence of the initial …

Einstein-Cartan gravity is a close historical sibling of general relativity that allows for
spacetime torsion. As a result, angular momentum couples to spacetime geometry in a …

We analyze the kinematics of cosmological spacetimes with nonzero torsion, in the
framework of the classical Einstein-Cartan gravity. After a brief introduction to the basic …

We derive asymptote solution of a homogeneous and isotropic universe governed by the
quadratic form of the field equation of f (T) gravity. We explain how the higher order of the …