Dark Energy, Hyperbolic Cosecant Cardassian and Virial Collapse for Power-style Cardassian
Wen-Jie Tian (SNNU)

TL;DR
This paper introduces a new hyperbolic cosecant Cardassian model within the GF fluid framework, analyzing its dynamical behavior, phase space, and virial collapse, demonstrating its stability and ability to facilitate virialization without singularities.
Contribution
It develops a novel hyperbolic cosecant Cardassian model with detailed dynamical analysis and explores virial collapse processes, highlighting stability and parameter effects.
Findings
Critical points exhibit self-consistency and auto-normalization.
Virial collapse of matter alone is forbidden, but possible with Cardassian effects.
No singularities are generated in the collapse process.
Abstract
New work gathers in Chapter 6 and Chapter 7. Tthe Cardassian dynamical equations are introduced generally and logically under GF fluid scenario, together with the flowing process of constructing phase space and differential dynamical systems from Friedmann equation. Hyperbolic cosecant Cardassian term is employed for concrete computing. The analysis proceeds in two cases, namely a unified description of matter and radiation energy density (case 1) and a separate description of matter and radiation terms (case 2).Formalism of case 2 is more exact at the expense of more complicatedness, and due to the mathematical symmetry of matter term and radiation term in hyperbolic cosecant function, the differential dynamical equations are considerably simplified. Phase space and dynamical systems for both cases are achieved. When we calculate the critical points for case 2, amazingly interesting…
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Taxonomy
TopicsAstro and Planetary Science · Cosmology and Gravitation Theories · Stellar, planetary, and galactic studies
