Time behavior of hubble parameter by torsion
- Consequences of the consistent exact solution of Einstein{Cartan equation on the time dependence of Hubble parameter are discussed. The torsion leads to a space and time-dependent expansion parameter which results into nontrivial windows of Hubble parameter between diverging behavior. Only one window shows a period of decreasing followed by increasing time dependence. Provided a known cosmological constant and the present values of Hubble and deceleration parameter this changing time can be given in the past as well as the ending time of the windows or universe. The comparison with the present experimental data allows to determine all parameters of the model. Large-scale spatial periodic structures appear. From the metric with torsion outside matter, it is seen that torsion can feign dark matter.
Author: | Klaus MorawetzORCiD |
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URN: | urn:nbn:de:hbz:836-opus-179736 |
DOI: | https://doi.org/10.25974/fhms-17973 |
DOI of original publication: | https://doi/org/10.1142/S0217732323501924 |
Parent Title (English): | Modern Physics Letters A |
Document Type: | Article |
Language: | English |
Date of Publication (online): | 2024/05/14 |
Year of first Publication: | 2024 |
Provider of the Publication Server: | FH Münster - University of Applied Sciences |
Release Date: | 2024/05/14 |
Tag: | Gravitation, Hubble constant, Cosmology, Torsion |
Volume: | Vol. 39 |
Issue: | No. 3 |
First Page: | 2350192-1 |
Last Page: | 2350192-10 |
Faculties: | Physikingenieurwesen (PHY) |
open_access (DINI-Set): | open_access |
Publication list: | Morawetz, Klaus |
Licence (German): | Creative Commons - Namensnennung - Nicht kommerziell - Keine Bearbeitungen 4.0 International (CC BY-NC-ND 4.0) |