Saved in:
| Main Authors: | , , |
|---|---|
| Format: | Recurso digital |
| Language: | |
| Published: |
Zenodo
2026
|
| Subjects: | |
| Online Access: | https://doi.org/10.5281/zenodo.19606278 |
| Tags: |
Add Tag
No Tags, Be the first to tag this record!
|
Table of Contents:
- <p class="FirstParagraph"><em><span>This research provides a rigorous analytical treatment of a spatially homogeneous Bianchi Type-III universe evolving under the influence of a Hoyle-Narlikar creation field (C-field). By integrating the modified Einstein Field Equations for a zero-pressure matter distribution, we identify a critical geometric constraint </span></em><span> </span><em><span>)</span></em><em><span> that necessitates the proportionality of the transverse scale factors, </span></em><span> </span><em><span>. We explore the late-time behaviour of this anisotropic system by employing a power-law expansion technique to solve the underlying gravitational field equations. Our results quantify the evolution of the expansion scalar, shear tensor, and the deceleration parameter, providing a numerical cross-check for the model's physical viability. The study demonstrates that the continuous matter-creation mechanism of the C-field effectively counteracts the expansionary dilution of energy density, offering a non-singular cosmological alternative that maintains a steady-state matter profile without requiring a cosmological constant.</span></em></p> <p class="MsoBodyText"> </p>