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Cosmological signatures of torsion and how to distinguish torsion from the dark sector
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Bolejko, K 
ORCID: 0000-0001-7402-3836, Cinus, M and Roukema, BF 2020
, 'Cosmological signatures of torsion and how to distinguish torsion from the dark sector'
, Physical Review D, vol. 101, no. 10
, pp. 1-12
, doi: 10.1103/PhysRevD.101.104046.
ORCID: 0000-0001-7402-3836, Cinus, M and Roukema, BF 2020
, 'Cosmological signatures of torsion and how to distinguish torsion from the dark sector'
, Physical Review D, vol. 101, no. 10
, pp. 1-12
, doi: 10.1103/PhysRevD.101.104046.
|
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Abstract
Torsion is a non-Riemannian geometrical extension of general relativity that allows including the spin of matter and the twisting of spacetime. Cosmological models with torsion have been considered in the literature to solve problems of either the very early (high redshift
| Item Type: | Article |
|---|---|
| Authors/Creators: | Bolejko, K and Cinus, M and Roukema, BF |
| Journal or Publication Title: | Physical Review D |
| Publisher: | American Physical Society |
| ISSN: | 2470-0010 |
| DOI / ID Number: | 10.1103/PhysRevD.101.104046 |
| Copyright Information: | © 2020 American Physical Society |
| Item Statistics: | View statistics for this item |
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