Theory of gravity with the Dirac scalar field and the problem of cosmological constant (Q1943792)
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scientific article; zbMATH DE number 6147543
| Language | Label | Description | Also known as |
|---|---|---|---|
| English | Theory of gravity with the Dirac scalar field and the problem of cosmological constant |
scientific article; zbMATH DE number 6147543 |
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Theory of gravity with the Dirac scalar field and the problem of cosmological constant (English)
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21 March 2013
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The authors use a Weyl-Cartan space, i.e., a space-time including torsion, to calculate the expansion of the universe in the presence of a Dirac scalar field. To this end they apply methods of quantum field theory. The same authors have already earlier discussed the Weyl-Cartan space, see [\textit{O. V. Baburova} et al., Russ. Phys. J. 54, No. 1, 121--123 (2011); translation from Izv. Vyssh. Uchebn. Zaved., Fiz., No. 1, 109--110 (2011; Zbl 1242.83085)]. Note: Due to an incorrect back-translation, the English language version of this paper contains the name Kartan, which should always read Cartan.
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Weyl-Cartan space
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Dirac scalar field
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torsion
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scalar field
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smological constant
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dark energy
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