Summary
We show that if one takes into account Penrose’s conformai technique in the Einstein-Cartan gravity, it is possible to obtain a relation between Hubble’s expansion and Birch’s rotation of the Universe at space-like infinity. This relation also leads to the final reduction of the gravitational coupling to a dimensionless quantity of order unity at space-like infinity. Initial-value equations at space-like infinity in the Einstein-Cartan gravity can be used as a starting point to study the structure formation and evolution of the Universe with Ω = 1. Current measurements of the expansion and rotation of the Universe favour the massive spinning particle as a candidate particle for dark matter.
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Palle, D. On certain relationships between cosmological observables in the Einstein-Cartan gravity. Nuov Cim B 111, 671–675 (1996). https://doi.org/10.1007/BF02743397
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DOI: https://doi.org/10.1007/BF02743397
PACS
- 04.50
- Gravity in more than four dimensions
- Kaluza-Klein theory
- unified field theories
- alternative theories of gravity