Cosmological Dark Matter Amplification through Dark Torsion
arXiv:2004.06058 · doi:10.1088/1361-6382/abb2d2
Abstract
A cosmological approach based on considering a cosmic background with non-zero torsion is shown in order to give an option of explaining a possible phantom evolution, not ruled out according to the current observational data. We revise some aspects of the formal schemes on torsion and, according them, we develop a formalism which can be an interesting alternative for exploring Cosmology.
arXiv comment10 pages
References in corpus (34)
- A direct empirical proof of the existence of dark matter
- Physical Aspects of the Space-Time Torsion
- Dark Matter and Dark Energy Interactions: Theoretical Challenges, Cosmological Implications and Observational Signatures
- Revealing the properties of dark matter in the merging cluster MACSJ0025.4-1222
- Observational information for f(T) theories and Dark Torsion
- Nonsingular, big-bounce cosmology from spinor-torsion coupling
- Consequences of Propagating Torsion in Connection-Dynamic Theories of Gravity
- Universe Generation from Black Hole Interiors
- Universe in a black hole in EinsteinCartan gravity
- Testing Generalized Einstein-Cartan-Kibble-Sciama Gravity using Weak Deflection Angle and Shadow Cast
- Friedmann-like universes with torsion
- On Poincaré gauge theory of gravity, its equations of motion, and Gravity Probe B
- The theory of local mass dimension one fermions of spin one half
- Nonsingular Dirac particles in spacetime with torsion
- Chern-Simons Forms in Gravitation Theories
- The cosmology of minimal varying Lambda theories
- Kinematics of Einstein-Cartan universes
- Elko and mass dimension one field of spin one half: causality and Fermi statistics
- Parity violating Friedmann Universes
- Cosmology with Scalar-Euler form Coupling
- Prospects of detecting spacetime torsion
- Non-minimally coupled scalar field cosmology with torsion
- Dark energy and Dark matter interaction in light of the second law of thermodynamics
- Nonminimal couplings, gravitational waves, and torsion in Horndeski's theory
- Non-parametric reconstruction of an inflaton potential from Einstein-Cartan-Sciama-Kibble gravity with particle production
- Non-zero torsion and late cosmology
- Gravity-induced four-fermion contact interaction implies gravitational intermediate W and Z type gauge bosons
- Acceleration in Friedmann cosmology with torsion
- Luminal Propagation of Gravitational Waves in Scalar-tensor Theories: The Case for Torsion
- Spacetime torsion as a possible remedy to major problems in gravity and cosmology
- The Spin Tensor of Dark Matter and the Hubble Parameter Tension
- Gravity waves in parity-violating Copernican Universes
- Einstein-Cartan-Dirac gravity with symmetry breaking
- The homogeneous and isotropic Weyssenhoff fluid