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Cosmological Dark Matter Amplification through Dark Torsion
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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.
Forward citations
Cited by 2 Pith papers
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Torsional pseudo-inflation beyond Einstein-Cartan
Spin-fluid torsion cannot sustain inflation beyond about 0.46 e-folds, but a coupling-fed axial torsion condensate can hold an exact de Sitter background with an algebraic exit.
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Quantum-Ordering Ambiguities in Weak Chern-Simons 4D Gravity and Metastability of the Condensate-Induced Inflation
In a Chern-Simons gravity model, quantum-ordering-dependent imaginary parts of the gravitational anomaly condensate give inflation a finite lifetime and imply the string scale is about one tenth of the Planck mass.
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