Phantom dark energy from scalar$-$torsion coupling
Nikodem J. Pop{\l}awski

TL;DR
This paper proposes a model where a scalar field coupled to torsion in Einstein-Cartan gravity acts as a source of phantom dark energy due to its negative kinetic term, offering a novel approach to dark energy modeling.
Contribution
It introduces a scalar-torsion coupling in Einstein-Cartan theory that results in a phantom dark energy candidate with a negative kinetic term.
Findings
Scalar field becomes kinetic through coupling to torsion.
The kinetic term is negative, indicating phantom dark energy behavior.
Provides a new theoretical framework for dark energy models.
Abstract
We show that a scalar field without a kinetic term in the Lagrangian density, coupled to the covariant divergence of the torsion vector in the EinsteinCartan theory of gravity, becomes kinetic in its general-relativistic equivalent formulation. The resulting kinetic term is negative: such a scalar field could be a source of phantom dark energy.
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