Exact Global Phantonical Solutions in the Emergent Universe
A. Beesham, S. V. Chervon, S. D. Maharaj, A. S. Kubasov

TL;DR
This paper introduces new exact solutions for an Emergent Universe model involving phantom and canonical scalar fields within a chiral cosmological framework, providing a detailed derivation method and cosmological parameter analysis.
Contribution
It presents a novel class of exact solutions for a phantonical Emergent Universe supported by scalar fields, expanding the theoretical understanding of such cosmological models.
Findings
Solutions are valid for all time
Detailed derivation method provided
Potential and kinetic interactions analyzed
Abstract
We present new classes of exact solutions for an Emergent Universe supported by phantom and canonical scalar fields in the framework of a two-component chiral cosmological model. We outline in detail the method of deriving exact solutions, discuss the potential and kinetic interaction for the model and calculate key cosmological parameters. We suggest that this this model be called a {\it phantonical Emergent Universe} because of the necessity to have phantom and canonical chiral fields. The solutions obtained are valid for all time.
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
Taxonomy
TopicsCosmology and Gravitation Theories · Black Holes and Theoretical Physics · Relativity and Gravitational Theory
