Tilted and Non Tilted C-Field Cosmological Models
D. D. Pawar, V. J. Dagwal, S. P. Shahare

TL;DR
This paper explores tilted and non-tilted homogeneous plane symmetric C-field cosmological models, analyzing their solutions, physical parameters, and universe evolution stages based on a specific creation field dependent on time.
Contribution
It presents new solutions for tilted and non-tilted C-field cosmological models using a method by Narlikar and Padmanabhan, with assumptions linking pressure and density.
Findings
Different stages of universe evolution are characterized in non-tilted models.
Physical parameters' behaviors are analyzed over cosmic time.
Deterministic models are derived with specific pressure-density relations.
Abstract
Tilted and non tilted homogeneous plane symmetric C-field cosmological models are investigated. Using the method of Narlikar and Padmanabhan [4], the solutions have been presented when the creation field C is function of time t only. To get the deterministic model, we have assumed the supplementary condition between pressure and density . The behaviour of different stages of the universe has been studied in non tilted models. We have also investigated the behaviours of some physical parameters.
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Taxonomy
TopicsCosmology and Gravitation Theories · Relativity and Gravitational Theory · Advanced Mathematical Theories and Applications
