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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.
1901
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1902
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1903
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J. Magueijo, T. Złośnik, Parity violating Friedmann Universes
1908
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J. Weyssenhoff, A. Raabe, Relativistic dynamics of spin-fluids and spin-particules
1947
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Y. Obukhov, V. Korotky, The Weyssenhoff fluid in Einstein-Cartan theory
1987
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2001
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D. Clowe, M. Bradac, A. González, M. Markevitch, S. Randall, C. Jones, D. Zaritsky, A direct empirical proof of the existence of dark matter
2006
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2008
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C. Boehmer, P. Bronowski, The homogeneous and isotropic Weyssenhoff fluid
2010
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D. Freedman, A. Van Proeyen, Supergravity
2012
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N. Popławski, Nonsingular, big-bounce cosmology from spinor-torsion coupling
2012
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K. Pasmatsiou, C. Tsagas, J. Barrow, Kinematics of Einstein-Cartan universes
2017
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2017
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2018
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S. Lepe and G. Otalora, Gauss–Bonnet dark energy on Hořava–Lifshitz cosmology,
2018
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D. Kranas, C. Tsagas, J. Barrow, D. Iosifidis, Friedmann-like universes with torsion
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2013
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2016
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Planck Collaboration, Planck Collaboration
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2019
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2019
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