Lorentzian Correction for the Evolution of the CMB Temperature.
Saved in:
| Title: | Lorentzian Correction for the Evolution of the CMB Temperature. |
|---|---|
| Authors: | Novais, A.1 (AUTHOR) arturnovais@gmail.com, Ribero, A. L. B.1 (AUTHOR) |
| Source: | Astrophysics. Sep2024, Vol. 67 Issue 3, p348-363. 16p. |
| Subjects: | Time dilation, Galaxy formation, Energy conservation, Spacetime, Physical cosmology |
| Abstract: | Observational evidence consistently shows that the universe is spatially flat and undergoes Lorentzian time dilation as a function of redshift. In combination, such discoveries suggest that a Minkowskian description of cosmology might be technically viable. The thermal evolution that transpires in a conformal spacetime is herein derived. The description is constrained by the energy conservation of a unified cosmic fluid. The resulting model puts forth a Lorentzian correction for the temperature of the CMB as a function of redshift, which improves current data fitting without adding any free parameter. Furthermore, it sheds light upon the early galaxy formation problem: our model predicts up to 0.86 Gyr older objects within the first two billion years of the structure evolution in the universe. [ABSTRACT FROM AUTHOR] |
| Copyright of Astrophysics is the property of Springer Nature and its content may not be copied or emailed to multiple sites without the copyright holder's express written permission. Additionally, content may not be used with any artificial intelligence tools or machine learning technologies. However, users may print, download, or email articles for individual use. This abstract may be abridged. No warranty is given about the accuracy of the copy. Users should refer to the original published version of the material for the full abstract. (Copyright applies to all Abstracts.) | |
| Database: | Engineering Source |
Be the first to leave a comment!